Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems | Paper Citation Record

Observation 388fa599-5273-4954-9bdd-729971c79652 · outbound

This paper cites doi:10.1007/978-3-642-30304-3 , adsurl =.

Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems doi:10.1007/978-3-642-30304-3 , adsurl =

Reference 1

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Observation 055df4ff-d8ec-42eb-a825-60349dd67955 · outbound

This paper cites The dependence of convective core overshooting on stellar mass: reality check, and additional evidence.

Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems The dependence of convective core overshooting on stellar mass: reality check, and additional evidence

Reference 2

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Observation fd0d35f1-e656-4807-9255-cb28a483a80f · outbound

This paper cites Significant uncertainties from calibrating overshooting with eclipsing binary systems.

Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems Significant uncertainties from calibrating overshooting with eclipsing binary systems

Reference 3

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Observation 6aada1b3-46ed-4dff-a206-69bb1aca81f0 · outbound

This paper cites Cepheids with giant companions. I. Revealing a numerous population of double-lined binary Cepheids.

Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems Cepheids with giant companions. I. Revealing a numerous population of double-lined binary Cepheids

Reference 4

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Observation 9791004a-2d08-4680-a019-b45216c0de86 · outbound

This paper cites an unresolved cited work.

Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems Unresolved cited work

Reference 5

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Observation 48225f8f-c6fa-4caa-ae33-3ef1caa9a7ee · outbound

This paper cites u ber die H \.

Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems u ber die H \

Reference 6

Resolution: verified exact; doi, observed 2026-08-12T14:37:35.931969Z

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Observation 659bfcbc-8609-404c-9c43-45d73e018c08 · outbound

This paper cites Testing Mass Loss in Large Magellanic Cloud Cepheids using Infrared and Optical Observations II. Predictions and Tests of the OGLE-III Fundamental-Mode Cepheids.

Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems Testing Mass Loss in Large Magellanic Cloud Cepheids using Infrared and Optical Observations II. Predictions and Tests of the OGLE-III Fundamental-Mode Cepheids

Reference 7

Resolution: unresolved; no resolver link, observed 2026-08-12T14:37:34.837245Z

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Observation 6ffca1bb-6f02-4fc1-9c5f-721af33dbb59 · outbound

This paper cites On the Enhancement of Mass Loss in Cepheids Due to Radial Pulsation. II. The Effect of Metallicity.

Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems On the Enhancement of Mass Loss in Cepheids Due to Radial Pulsation. II. The Effect of Metallicity

Reference 8

Resolution: unresolved; no resolver link, observed 2026-08-12T14:37:34.842514Z

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Observation aafe628d-d07e-41c4-9bc4-b18d4a30d1ad · outbound

This paper cites Testing Mass Loss in Large Magellanic Cloud Cepheids using Infrared and Optical Observations.

Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems Testing Mass Loss in Large Magellanic Cloud Cepheids using Infrared and Optical Observations

Reference 9

Resolution: unresolved; no resolver link, observed 2026-08-12T14:37:34.847256Z

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Observation 4cc967b2-6e3d-4fe7-9bb9-d2a35cc7b23d · outbound

This paper cites On the Enhancement of Mass Loss in Cepheids Due to Radial Pulsation.

Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems On the Enhancement of Mass Loss in Cepheids Due to Radial Pulsation

Reference 10

Resolution: unresolved; no resolver link, observed 2026-08-12T14:37:34.852063Z

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Observation 0156e42a-f3a2-42bc-a784-a602cbc28fe8 · outbound

This paper cites The Cepheid mass discrepancy and pulsation-driven mass loss.

Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems The Cepheid mass discrepancy and pulsation-driven mass loss

Reference 11

Resolution: unresolved; no resolver link, observed 2026-08-12T14:37:34.856737Z

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Observation 01b96ff5-3185-4d5d-9d89-023fabafbec3 · outbound

This paper cites Stellar Pulsation and Evolution: a Combined Theoretical Renewal and Updated Models (SPECTRUM) -- I: Updating radiative opacities for pulsation models of Classical Cepheid and RR-Lyrae.

Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems Stellar Pulsation and Evolution: a Combined Theoretical Renewal and Updated Models (SPECTRUM) -- I: Updating radiative opacities for pulsation models of Classical Cepheid and RR-Lyrae

Reference 12

Resolution: unresolved; no resolver link, observed 2026-08-12T14:37:34.862071Z

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Observation 8f3b43ec-dab4-4085-9df0-16266c6b7d1a · outbound

This paper cites Models fitted to evolutionary tracks.

Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems Models fitted to evolutionary tracks

Reference 13

Resolution: unresolved; no resolver link, observed 2026-08-12T14:37:34.868081Z

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Observation d7fdcaf4-3bdf-4461-8f58-682677f20019 · outbound

This paper cites Models fitted to a new mass-luminosity relation.

Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems Models fitted to a new mass-luminosity relation

Reference 14

Resolution: verified exact; doi, observed 2026-08-12T14:37:35.905317Z

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Observation 3c117d6e-1596-48d5-b5e9-06052c2a8a5b · outbound

This paper cites an unresolved cited work.

Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems Unresolved cited work

Reference 15

Resolution: unresolved; no resolver link, observed 2026-08-12T14:37:34.878520Z

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Observation 6caa13f8-ed50-4890-b69f-322a3d0bceb1 · outbound

This paper cites Using classical Cepheids to study the far side of the Milky Way disk. II. The spiral structure in the first and fourth Galactic quadrants.

Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems Using classical Cepheids to study the far side of the Milky Way disk. II. The spiral structure in the first and fourth Galactic quadrants

Reference 16

Resolution: unresolved; no resolver link, observed 2026-08-12T14:37:34.883828Z

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Observation de4c61b7-3d9f-440b-b030-0317bf8ed2a5 · outbound

This paper cites OGLE-ing the Magellanic System: Cepheids in the Bridge.

Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems OGLE-ing the Magellanic System: Cepheids in the Bridge

Reference 17

Resolution: unresolved; no resolver link, observed 2026-08-12T14:37:34.889110Z

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Observation e9577f31-41a6-40f7-a5f7-f57588403f21 · outbound

This paper cites OGLE-ing the Magellanic System: Three-Dimensional Structure of the Clouds and the Bridge Using Classical Cepheids.

Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems OGLE-ing the Magellanic System: Three-Dimensional Structure of the Clouds and the Bridge Using Classical Cepheids

Reference 18

Resolution: unresolved; no resolver link, observed 2026-08-12T14:37:34.894008Z

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Observation da9ad911-7749-48ff-a4b5-5f4952a03200 · outbound

This paper cites Final Results from the Hubble Space Telescope Key Project to Measure the Hubble Constant.

Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems Final Results from the Hubble Space Telescope Key Project to Measure the Hubble Constant

Reference 19

Resolution: unresolved; no resolver link, observed 2026-08-12T14:37:34.898321Z

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Observation 777bc6e1-8edc-42b6-aab3-c55678a4288b · outbound

This paper cites , keywords =.

Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems , keywords =

Reference 20

Resolution: unresolved; no resolver link, observed 2026-08-12T14:37:34.902522Z

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Observation 9f480c9f-7790-4f10-ae4c-45aae21a42b7 · outbound

This paper cites , keywords =.

Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems , keywords =

Reference 21

Resolution: unresolved; no resolver link, observed 2026-08-12T14:37:34.906719Z

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Observation 34a3a622-91ea-4146-8ed1-2c6e19dc83e2 · outbound

This paper cites Origin and Evolution of the Elements , year = 1993, editor =.

Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems Origin and Evolution of the Elements , year = 1993, editor =

Reference 22

Resolution: unresolved; no resolver link, observed 2026-08-12T14:37:34.910618Z

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Observation 0e174198-c445-46e7-b123-8ad79cd0f30a · outbound

This paper cites , keywords =.

Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems , keywords =

Reference 23

Resolution: unresolved; no resolver link, observed 2026-08-12T14:37:34.915187Z

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Observation c68b31d0-7cfd-448d-8597-70a67cfebd07 · outbound

This paper cites Convective hydrocodes for radial stellar pulsation. Physical and numerical formulation.

Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems Convective hydrocodes for radial stellar pulsation. Physical and numerical formulation

Reference 24

Resolution: unresolved; no resolver link, observed 2026-08-12T14:37:34.919619Z

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Observation 078ca03b-cfd6-4e89-985f-f782f707e999 · outbound

This paper cites an unresolved cited work.

Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems Unresolved cited work

Reference 25

Resolution: unresolved; no resolver link, observed 2026-08-12T14:37:34.925142Z

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Observation c2d5dbc2-866e-4c51-9ca8-1c6346344d26 · outbound

This paper cites an unresolved cited work.

Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems Unresolved cited work

Reference 26

Resolution: unresolved; no resolver link, observed 2026-08-12T14:37:34.929540Z

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Observation 1d1feecd-a9d0-4b86-8a9e-d0d31b3df985 · outbound

This paper cites The NextGen Model Atmosphere grid: II. Spherically symmetric model atmospheres for giant stars with effective temperatures between 3000 and 6800~K.

Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems The NextGen Model Atmosphere grid: II. Spherically symmetric model atmospheres for giant stars with effective temperatures between 3000 and 6800~K

Reference 27

Resolution: unresolved; no resolver link, observed 2026-08-12T14:37:34.934862Z

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Observation 7a57f46e-43cf-4aae-8975-5a95db662889 · outbound

This paper cites The NextGen Model Atmosphere grid for $3000\le \Teff \le 10000\K$.

Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems The NextGen Model Atmosphere grid for $3000\le \Teff \le 10000\K$

Reference 28

Resolution: unresolved; no resolver link, observed 2026-08-12T14:37:34.939594Z

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Observation 5a552c5a-fad6-423a-a02f-ede2cf9d1c83 · outbound

This paper cites , keywords =.

Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems , keywords =

Reference 29

Resolution: unresolved; no resolver link, observed 2026-08-12T14:37:34.944649Z

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Observation 19ae4c0f-5807-4af0-82df-9fcc176bac0f · outbound

This paper cites , keywords =.

Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems , keywords =

Reference 30

Resolution: unresolved; no resolver link, observed 2026-08-12T14:37:34.948913Z

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Observation 0b2472eb-e6e7-4b2e-94b7-2531f4db28d0 · outbound

This paper cites , keywords =.

Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems , keywords =

Reference 31

Resolution: unresolved; no resolver link, observed 2026-08-12T14:37:34.953340Z

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Observation e65985db-e721-4265-9665-ab3f912c2f1c · outbound

This paper cites Equation of state of fully ionized electron-ion plasmas. II. Extension to relativistic densities and to the solid phase.

Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems Equation of state of fully ionized electron-ion plasmas. II. Extension to relativistic densities and to the solid phase

Reference 32

Resolution: unresolved; no resolver link, observed 2026-08-12T14:37:34.957808Z

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Observation f5b19555-7a1b-4360-82f9-0a1d516efc79 · outbound

This paper cites Thermodynamic functions of dense plasmas: analytic approximations for astrophysical applications.

Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems Thermodynamic functions of dense plasmas: analytic approximations for astrophysical applications

Reference 33

Resolution: unresolved; no resolver link, observed 2026-08-12T14:37:34.962297Z

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Observation d09f4300-c3f9-407e-81df-81d9ecc7b192 · outbound

This paper cites A new equation of state for dense hydrogen-helium mixtures.

Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems A new equation of state for dense hydrogen-helium mixtures

Reference 34

Resolution: unresolved; no resolver link, observed 2026-08-12T14:37:34.967056Z

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Observation edccb19d-f29c-4361-b27b-a7032302307f · outbound

This paper cites Skye: A Differentiable Equation of State.

Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems Skye: A Differentiable Equation of State

Reference 35

Resolution: unresolved; no resolver link, observed 2026-08-12T14:37:34.971887Z

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Observation 566b221f-ddb6-4cbf-87ae-b7186924cc78 · outbound

This paper cites Low Temperature Opacities.

Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems Low Temperature Opacities

Reference 36

Resolution: unresolved; no resolver link, observed 2026-08-12T14:37:34.976780Z

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Observation 7247281c-6026-4028-8cb1-c1ee60da3c39 · outbound

This paper cites , keywords =.

Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems , keywords =

Reference 37

Resolution: unresolved; no resolver link, observed 2026-08-12T14:37:34.981844Z

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Observation a97bb179-9f51-4e0c-a474-02d88e3262c6 · outbound

This paper cites , keywords =.

Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems , keywords =

Reference 38

Resolution: unresolved; no resolver link, observed 2026-08-12T14:37:34.986415Z

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Observation f65652ac-661a-4b81-9fc7-5eb291c12973 · outbound

This paper cites , keywords =.

Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems , keywords =

Reference 39

Resolution: unresolved; no resolver link, observed 2026-08-12T14:37:34.990916Z

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Observation 6130c6f9-feb4-4e46-8453-805a5b370a50 · outbound

This paper cites The VMC survey -- XLIV: Mapping metallicity trends in the Large Magellanic Cloud using near-infrared passbands.

Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems The VMC survey -- XLIV: Mapping metallicity trends in the Large Magellanic Cloud using near-infrared passbands

Reference 40

Resolution: unresolved; no resolver link, observed 2026-08-12T14:37:34.995159Z

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Observation dc5a1f44-de1e-435e-84ab-17b2ab029f43 · outbound

This paper cites EAS Publications Series , year = 2009, editor =.

Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems EAS Publications Series , year = 2009, editor =

Reference 41

Resolution: unresolved; no resolver link, observed 2026-08-12T14:37:34.999585Z

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Observation 6655e22f-d4c7-4a15-a4ff-06687b48497a · outbound

This paper cites The Araucaria Project: The First-Overtone Classical Cepheid in the Eclipsing System OGLE-LMC-CEP-2532.

Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems The Araucaria Project: The First-Overtone Classical Cepheid in the Eclipsing System OGLE-LMC-CEP-2532

Reference 42

Resolution: unresolved; no resolver link, observed 2026-08-12T14:37:35.003639Z

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Observation 943750f2-63ff-4c36-8e37-72d6fe0844fb · outbound

This paper cites , keywords =.

Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems , keywords =

Reference 43

Resolution: unresolved; no resolver link, observed 2026-08-12T14:37:35.007854Z

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Observation 2da65194-863c-44d1-9c4d-76153b7bf63b · outbound

This paper cites A Classical Cepheid in a LMC eclipsing binary: evidence of shortcomings in current stellar evolutionary models?.

Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems A Classical Cepheid in a LMC eclipsing binary: evidence of shortcomings in current stellar evolutionary models?

Reference 44

Resolution: unresolved; no resolver link, observed 2026-08-12T14:37:35.011852Z

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Observation e4de3f36-0062-4224-87c7-74f281a5c211 · outbound

This paper cites A three-dimensional map of the Milky Way using classical Cepheid variable stars.

Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems A three-dimensional map of the Milky Way using classical Cepheid variable stars

Reference 45

Resolution: unresolved; no resolver link, observed 2026-08-12T14:37:35.016191Z

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Observation 8cb336df-83fc-49f8-badc-7684b503d9e4 · outbound

This paper cites Large Magellanic Cloud Cepheid Standards Provide a 1% Foundation for the Determination of the Hubble Constant and Stronger Evidence for Physics Beyond LambdaCDM.

Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems Large Magellanic Cloud Cepheid Standards Provide a 1% Foundation for the Determination of the Hubble Constant and Stronger Evidence for Physics Beyond LambdaCDM

Reference 46

Resolution: unresolved; no resolver link, observed 2026-08-12T14:37:35.020886Z

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Observation 092712c2-85e8-4204-b05f-b21f4550bde3 · outbound

This paper cites Harvard College Observatory Circular , year = 1912, month = mar, volume =.

Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems Harvard College Observatory Circular , year = 1912, month = mar, volume =

Reference 47

Resolution: unresolved; no resolver link, observed 2026-08-12T14:37:35.025694Z

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Observation fc4bf47f-733d-4e00-af8a-91c6cbcda7bf · outbound

This paper cites Annals of Harvard College Observatory , year = 1907, month = jan, volume =.

Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems Annals of Harvard College Observatory , year = 1907, month = jan, volume =

Reference 48

Resolution: unresolved; no resolver link, observed 2026-08-12T14:37:35.030097Z

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Observation 83070b95-7e8b-4518-9a87-8364cded0fa6 · outbound

This paper cites The Araucaria Project. OGLE-LMC-CEP-1718: An exotic eclipsing binary system composed of two classical overtone Cepheids in a 413-day orbit.

Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems The Araucaria Project. OGLE-LMC-CEP-1718: An exotic eclipsing binary system composed of two classical overtone Cepheids in a 413-day orbit

Reference 49

Resolution: unresolved; no resolver link, observed 2026-08-12T14:37:35.034400Z

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Observation eb2528e9-de55-4a67-9f9d-8b60f3b837fe · outbound

This paper cites Is there a mass discrepancy in the Cepheid binary OGLE-LMC-CEP0227?.

Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems Is there a mass discrepancy in the Cepheid binary OGLE-LMC-CEP0227?

Reference 50

Resolution: unresolved; no resolver link, observed 2026-08-12T14:37:35.039141Z

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Observation 0e9f0ec3-37b6-4485-a866-b4d95d00d11d · outbound

This paper cites Discovery of a binary-origin classical Cepheid in a binary system with a 59-day orbital period.

Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems Discovery of a binary-origin classical Cepheid in a binary system with a 59-day orbital period

Reference 51

Resolution: unresolved; no resolver link, observed 2026-08-12T14:37:35.043779Z

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Observation 509b3c1f-777a-4baa-9168-1934209a9207 · outbound

This paper cites A novel q-PED method: precise physical properties of a merger-origin binary Cepheid OGLE-LMC-CEP-1347.

Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems A novel q-PED method: precise physical properties of a merger-origin binary Cepheid OGLE-LMC-CEP-1347

Reference 52

Resolution: unresolved; no resolver link, observed 2026-08-12T14:37:35.048332Z

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Observation 94973cf3-bfe5-4a6c-97b9-d517e7cdfc73 · outbound

This paper cites The strange evolution of the Large Magellanic Cloud Cepheid OGLE-LMC-CEP1812.

Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems The strange evolution of the Large Magellanic Cloud Cepheid OGLE-LMC-CEP1812

Reference 53

Resolution: unresolved; no resolver link, observed 2026-08-12T14:37:35.053316Z

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Observation d9dca0c9-aa6e-42b6-8359-173c1dfed77f · outbound

This paper cites The Araucaria Project. Accurate determination of the dynamical mass of the classical Cepheid in the eclipsing system OGLE-LMC-CEP-1812.

Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems The Araucaria Project. Accurate determination of the dynamical mass of the classical Cepheid in the eclipsing system OGLE-LMC-CEP-1812

Reference 54

Resolution: verified exact; local_arxiv, observed 2026-08-12T14:37:37.024278Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

Observation 66a459dc-4f8e-4f91-b8fd-8eefa1b97d67 · outbound

This paper cites Physical parameters and the projection factor of the classical Cepheid in the binary system OGLE-LMC-CEP-0227.

Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems Physical parameters and the projection factor of the classical Cepheid in the binary system OGLE-LMC-CEP-0227

Reference 55

Resolution: verified exact; local_arxiv, observed 2026-08-12T14:37:37.003313Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

Observation 9c80ba6f-532a-42ff-968a-c8db8e92b34e · outbound

This paper cites The OGLE Collection of Variable Stars. Classical Cepheids in the Magellanic System.

Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems The OGLE Collection of Variable Stars. Classical Cepheids in the Magellanic System

Reference 56

Resolution: unresolved; no resolver link, observed 2026-08-12T14:37:35.066976Z

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Observation 6b0a3e98-2306-4196-990c-2e61abf60042 · outbound

This paper cites Multi-Mode and Non-Standard Classical Cepheids in the Magellanic System.

Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems Multi-Mode and Non-Standard Classical Cepheids in the Magellanic System

Reference 57

Resolution: verified exact; local_arxiv, observed 2026-08-12T14:37:35.753975Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

Observation 4edfb45d-338a-4be9-b21f-eb1491d10bff · outbound

This paper cites On the Effect of Rotation on Populations of Classical Cepheids II. Pulsation Analysis for Metallicities 0.014, 0.006, and 0.002.

Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems On the Effect of Rotation on Populations of Classical Cepheids II. Pulsation Analysis for Metallicities 0.014, 0.006, and 0.002

Reference 58

Resolution: unresolved; no resolver link, observed 2026-08-12T14:37:35.076596Z

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Unavailable: canonical work link unavailable.

Observation 5fa800a8-b3a9-49bb-a197-d76a62d43d4c · outbound

This paper cites On the effect of rotation on populations of classical Cepheids I. Predictions at solar metallicity.

Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems On the effect of rotation on populations of classical Cepheids I. Predictions at solar metallicity

Reference 59

Resolution: unresolved; no resolver link, observed 2026-08-12T14:37:35.081283Z

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Unavailable: canonical work link unavailable.

Observation d8eed683-ebdf-47aa-a623-9c6463101050 · outbound

This paper cites Cepheid Mass-loss and the Pulsation -- Evolutionary Mass Discrepancy.

Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems Cepheid Mass-loss and the Pulsation -- Evolutionary Mass Discrepancy

Reference 60

Resolution: verified exact; local_arxiv, observed 2026-08-12T14:37:36.949661Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

Observation 77e2da00-d8e2-469e-a97a-756a80924d1e · outbound

This paper cites , keywords =.

Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems , keywords =

Reference 61

Resolution: unresolved; no resolver link, observed 2026-08-12T14:37:35.090827Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e4aaebf1-b30d-45ed-a1cc-3dec251865f8 · outbound

This paper cites , keywords =.

Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems , keywords =

Reference 62

Resolution: unresolved; no resolver link, observed 2026-08-12T14:37:35.095077Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 67463b42-22d1-4f61-b5c1-390308691fed · outbound

This paper cites , keywords =.

Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems , keywords =

Reference 63

Resolution: unresolved; no resolver link, observed 2026-08-12T14:37:35.099548Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 646347c6-246a-433c-b085-e5f7018f4cd3 · outbound

This paper cites , year = 1968, month = mar, volume =.

Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems , year = 1968, month = mar, volume =

Reference 64

Resolution: unresolved; no resolver link, observed 2026-08-12T14:37:35.103637Z

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Unavailable: canonical work link unavailable.

Observation b8f3b82b-77c2-45da-8d08-d0f81ce8b870 · outbound

This paper cites On the evolutionary and pulsation mass of Classical Cepheids: III. the case of the eclipsing binary Cepheid CEP0227 in the Large Magellanic Cloud.

Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems On the evolutionary and pulsation mass of Classical Cepheids: III. the case of the eclipsing binary Cepheid CEP0227 in the Large Magellanic Cloud

Reference 65

Resolution: verified exact; local_arxiv, observed 2026-08-12T14:37:36.855070Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

Observation e8fc5723-b49f-4d1c-a980-b6fc9b3526ec · outbound

This paper cites Accurate dynamical mass determination of a classical Cepheid in an eclipsing binary system.

Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems Accurate dynamical mass determination of a classical Cepheid in an eclipsing binary system

Reference 66

Resolution: unresolved; no resolver link, observed 2026-08-12T14:37:35.113015Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ce4bef51-53e1-40a6-bb35-a785742d6660 · outbound

This paper cites Luminosities and mass-loss rates of SMC and LMC AGB stars and Red Supergiants.

Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems Luminosities and mass-loss rates of SMC and LMC AGB stars and Red Supergiants

Reference 67

Resolution: verified exact; local_arxiv, observed 2026-08-12T14:37:36.821378Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

Observation 99587992-8ad3-43cd-953a-aa35b3d3ae95 · outbound

This paper cites Connecting integrated RGB mass loss from asteroseismology and globular clusters.

Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems Connecting integrated RGB mass loss from asteroseismology and globular clusters

Reference 68

Resolution: verified exact; local_arxiv, observed 2026-08-12T14:37:36.801531Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

Observation 5bfeb0b8-8935-40e8-9a94-bb7bcb6b8301 · outbound

This paper cites Asteroseismic Study of Subgiants and Giants of the Open Cluster M67 using Kepler/K2: Expanded Sample and Precise Masses.

Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems Asteroseismic Study of Subgiants and Giants of the Open Cluster M67 using Kepler/K2: Expanded Sample and Precise Masses

Reference 69

Resolution: verified exact; local_arxiv, observed 2026-08-12T14:37:36.780333Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

Observation 757d5341-6e4c-4a70-beb8-b76073a95a18 · outbound

This paper cites Theoretical investigation on the mass loss impact on asteroseismic grid-based estimates of mass, radius, and age for RGB stars.

Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems Theoretical investigation on the mass loss impact on asteroseismic grid-based estimates of mass, radius, and age for RGB stars

Reference 70

Resolution: verified exact; local_arxiv, observed 2026-08-12T14:37:36.759106Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

Observation c3fef32c-35fa-4ba7-96fa-8418432c6138 · outbound

This paper cites an unresolved cited work.

Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems Unresolved cited work

Reference 71

Resolution: unresolved; no resolver link, observed 2026-08-12T14:37:35.137548Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a3e9d900-29e4-4352-8fb6-6fb81e98cdd5 · outbound

This paper cites Memoires of the Societe Royale des Sciences de Liege , keywords =.

Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems Memoires of the Societe Royale des Sciences de Liege , keywords =

Reference 72

Resolution: unresolved; no resolver link, observed 2026-08-12T14:37:35.142043Z

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Unavailable: canonical work link unavailable.

Observation 613ed5f9-41c2-41e9-88b6-51164e484018 · outbound

This paper cites The evolution of AGB stars with convective overshoot.

Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems The evolution of AGB stars with convective overshoot

Reference 73

Resolution: unresolved; no resolver link, observed 2026-08-12T14:37:35.146531Z

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Unavailable: canonical work link unavailable.

Observation 37a707d7-acd7-4288-8063-72b39e1ae53e · outbound

This paper cites New Grids of ATLAS9 Model Atmospheres.

Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems New Grids of ATLAS9 Model Atmospheres

Reference 74

Resolution: unresolved; no resolver link, observed 2026-08-12T14:37:35.151320Z

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Unavailable: canonical work link unavailable.

Observation 2df42163-618b-43b9-96f2-723a92059b07 · outbound

This paper cites Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation.

Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation

Reference 75

Resolution: unresolved; no resolver link, observed 2026-08-12T14:37:35.155970Z

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Unavailable: canonical work link unavailable.

Observation 88f82d53-56be-48e8-a5aa-51f14e4f266a · outbound

This paper cites Modules for Experiments in Stellar Astrophysics (MESA): Time-Dependent Convection, Energy Conservation, Automatic Differentiation, and Infrastructure.

Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems Modules for Experiments in Stellar Astrophysics (MESA): Time-Dependent Convection, Energy Conservation, Automatic Differentiation, and Infrastructure

Reference 76

Resolution: unresolved; no resolver link, observed 2026-08-12T14:37:35.160675Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 57c5be9c-bf41-4996-9bce-aa31bde45f24 · outbound

This paper cites Modules for Experiments in Stellar Astrophysics (MESA): Pulsating Variable Stars, Rotation, Convective Boundaries, and Energy Conservation.

Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems Modules for Experiments in Stellar Astrophysics (MESA): Pulsating Variable Stars, Rotation, Convective Boundaries, and Energy Conservation

Reference 77

Resolution: unresolved; no resolver link, observed 2026-08-12T14:37:35.165434Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a3c1d7b2-b2de-4d72-b225-1ea1f2adbfd3 · outbound

This paper cites Modules for Experiments in Stellar Astrophysics (MESA): Convective Boundaries, Element Diffusion, and Massive Star Explosions.

Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems Modules for Experiments in Stellar Astrophysics (MESA): Convective Boundaries, Element Diffusion, and Massive Star Explosions

Reference 78

Resolution: unresolved; no resolver link, observed 2026-08-12T14:37:35.171133Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 1cac9454-03f6-4941-9a04-81aa791765e0 · outbound

This paper cites , year = 2016, month = mar, volume =.

Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems , year = 2016, month = mar, volume =

Reference 79

Resolution: unresolved; no resolver link, observed 2026-08-12T14:37:35.175797Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 684bed69-d383-4ea0-886f-3fd54576186f · outbound

This paper cites Modules for Experiments in Stellar Astrophysics (MESA): Binaries, Pulsations, and Explosions.

Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems Modules for Experiments in Stellar Astrophysics (MESA): Binaries, Pulsations, and Explosions

Reference 80

Resolution: unresolved; no resolver link, observed 2026-08-12T14:37:35.180862Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d0128cb6-aed4-4308-8057-9f25fb696713 · outbound

This paper cites Modules for Experiments in Stellar Astrophysics (MESA): Giant Planets, Oscillations, Rotation, and Massive Stars.

Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems Modules for Experiments in Stellar Astrophysics (MESA): Giant Planets, Oscillations, Rotation, and Massive Stars

Reference 81

Resolution: unresolved; no resolver link, observed 2026-08-12T14:37:35.185749Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 4929153d-7f1b-479b-8eac-6ab4705fa6ae · outbound

This paper cites Modules for Experiments in Stellar Astrophysics (MESA).

Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems Modules for Experiments in Stellar Astrophysics (MESA)

Reference 82

Resolution: unresolved; no resolver link, observed 2026-08-12T14:37:35.190062Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 038b2d84-0c21-40e6-a583-8e99eb970b08 · outbound

This paper cites Toward a Comprehensive Grid of Cepheid Models with MESA I. Uncertainties of the Evolutionary Tracks of Intermediate-Mass Stars.

Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems Toward a Comprehensive Grid of Cepheid Models with MESA I. Uncertainties of the Evolutionary Tracks of Intermediate-Mass Stars

Reference 83

Resolution: verified exact; local_arxiv, observed 2026-08-12T14:37:36.635485Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

Observation 445f2d2e-9b95-4fa9-a03e-713c713b542f · outbound

This paper cites , keywords =.

Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems , keywords =

Reference 84

Resolution: unresolved; no resolver link, observed 2026-08-12T14:37:35.198578Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation b0f910e6-939f-4d6e-8e6e-24672410cb40 · outbound

This paper cites The Optical Gravitational Lensing Experiment. The OGLE-III Catalog of Variable Stars. I. Classical Cepheids in the Large Magellanic Cloud.

Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems The Optical Gravitational Lensing Experiment. The OGLE-III Catalog of Variable Stars. I. Classical Cepheids in the Large Magellanic Cloud

Reference 85

Resolution: unresolved; no resolver link, observed 2026-08-12T14:37:35.202981Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 7bc2a729-6ba2-4025-ba82-73b81b9ae4cd · outbound

This paper cites Non-radial modes in classical Cepheids. What to look for in spectroscopy?.

Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems Non-radial modes in classical Cepheids. What to look for in spectroscopy?

Reference 86

Resolution: verified exact; local_arxiv, observed 2026-08-12T14:37:36.533759Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

Observation b7c3a8af-5b71-4047-82c7-30b036b94669 · outbound

This paper cites Candidates for non-pulsating stars located in the Cepheid instability strip in the Large Magellanic Cloud based on Str\"omgren photometry.

Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems Candidates for non-pulsating stars located in the Cepheid instability strip in the Large Magellanic Cloud based on Str\"omgren photometry

Reference 87

Resolution: verified exact; local_arxiv, observed 2026-08-12T14:37:36.513599Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

Observation 408ec0d3-b229-4cd6-9990-50063a4535f2 · outbound

This paper cites Stellar Populations and the Distance Scale , year = 2018, editor =.

Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems Stellar Populations and the Distance Scale , year = 2018, editor =

Reference 88

Resolution: unresolved; no resolver link, observed 2026-08-12T14:37:35.216774Z

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Unavailable: canonical work link unavailable.

Observation 0a682472-bb11-41d7-b684-18bcff1d68ff · outbound

This paper cites Eclipsing Binaries with Classical Cepheid Component in the Magellanic System.

Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems Eclipsing Binaries with Classical Cepheid Component in the Magellanic System

Reference 89

Resolution: unresolved; no resolver link, observed 2026-08-12T14:37:35.221244Z

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Unavailable: canonical work link unavailable.

Observation 0c146459-a989-44b7-93db-88d317930e1e · outbound

This paper cites Observational calibration of the projection factor of Cepheids IV. Period-projection factor relation of Galactic and Magellanic Cloud Cepheids.

Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems Observational calibration of the projection factor of Cepheids IV. Period-projection factor relation of Galactic and Magellanic Cloud Cepheids

Reference 90

Resolution: unresolved; no resolver link, observed 2026-08-12T14:37:35.225864Z

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Observation 6010608d-5c50-4f11-829b-b8245ca32179 · outbound

This paper cites The influential effect of blending, bump, changing period and eclipsing Cepheids on the Leavitt law.

Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems The influential effect of blending, bump, changing period and eclipsing Cepheids on the Leavitt law

Reference 91

Resolution: verified exact; local_arxiv, observed 2026-08-12T14:37:36.477853Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

Observation e682bfa1-9298-4fff-9c76-f0f29f59474d · outbound

This paper cites The Optical Gravitational Lensing Experiment. Gaia South Ecliptic Pole Field as Seen by OGLE-IV.

Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems The Optical Gravitational Lensing Experiment. Gaia South Ecliptic Pole Field as Seen by OGLE-IV

Reference 92

Resolution: verified exact; local_arxiv, observed 2026-08-12T14:37:35.642534Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

Observation ef6bd687-7f29-4f32-b0f4-d047d527af04 · outbound

This paper cites The Araucaria Project: A study of the classical Cepheid in the eclipsing binary system OGLE LMC562.05.9009 in the Large Magellanic Cloud.

Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems The Araucaria Project: A study of the classical Cepheid in the eclipsing binary system OGLE LMC562.05.9009 in the Large Magellanic Cloud

Reference 93

Resolution: verified exact; local_arxiv, observed 2026-08-12T14:37:36.458410Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

Observation 4086704e-f013-4bb5-a1d8-06ddadeb39ef · outbound

This paper cites Period Change Rates in Large Magellanic Cloud Cepheids Revisited.

Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems Period Change Rates in Large Magellanic Cloud Cepheids Revisited

Reference 94

Resolution: verified exact; local_arxiv, observed 2026-08-12T14:37:36.438240Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

Observation d58bbe07-d918-488e-be4d-b33b8a23ed7b · outbound

This paper cites Non-evolutionary effects on period change in Magellanic Cepheids II. Empirical constraints on non-linear period changes.

Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems Non-evolutionary effects on period change in Magellanic Cepheids II. Empirical constraints on non-linear period changes

Reference 95

Resolution: verified exact; local_arxiv, observed 2026-08-12T14:37:36.417036Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

Observation 5030e462-9765-4263-a244-5940e0610e1f · outbound

This paper cites Non-evolutionary effects on period change in Magellanic Cepheids I. New binary systems revealed from Light Travel Time Effect.

Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems Non-evolutionary effects on period change in Magellanic Cepheids I. New binary systems revealed from Light Travel Time Effect

Reference 96

Resolution: verified exact; local_arxiv, observed 2026-08-12T14:37:36.395478Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

Observation 348c7c9c-f957-476a-ac9b-924b28e423f0 · outbound

This paper cites The iron and oxygen content of LMC Classical Cepheids and its implications for the Extragalactic Distance Scale and Hubble constant.

Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems The iron and oxygen content of LMC Classical Cepheids and its implications for the Extragalactic Distance Scale and Hubble constant

Reference 97

Resolution: unresolved; no resolver link, observed 2026-08-12T14:37:35.259005Z

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Unavailable: canonical work link unavailable.

Observation a6756497-e59a-474f-a2b9-b1cf63ca1f48 · outbound

This paper cites Metallicity estimation of MW, SMC and LMC classical Cepheids from the shape of the $V$- and $I$-band light curves.

Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems Metallicity estimation of MW, SMC and LMC classical Cepheids from the shape of the $V$- and $I$-band light curves

Reference 98

Resolution: verified exact; local_arxiv, observed 2026-08-12T14:37:36.358010Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

Observation c030acd2-cbe5-4b9c-a5fb-1ef4836b51d4 · outbound

This paper cites Implications of a turbulent convection model for classical Cepheids.

Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems Implications of a turbulent convection model for classical Cepheids

Reference 99

Resolution: verified exact; local_arxiv, observed 2026-08-12T14:37:36.337006Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

Observation c03b01de-1f99-4259-8e2c-3a91ad970cb7 · outbound

This paper cites The Araucaria Project: High-precision Cepheid astrophysics from the analysis of variables in double-lined eclipsing binaries.

Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems The Araucaria Project: High-precision Cepheid astrophysics from the analysis of variables in double-lined eclipsing binaries

Reference 100

Resolution: unresolved; no resolver link, observed 2026-08-12T14:37:35.274600Z

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