Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations | Paper Citation Record

Observation 8c47027b-89a7-4a2b-979c-02d1a198a3c7 · outbound

This paper cites , " * write output.state after.block = add.period write newline.

Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations , " * write output.state after.block = add.period write newline

Reference 1

Resolution: unresolved; no resolver link, observed 2026-08-05T10:57:04.454177Z

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Observation 274dff59-38ce-46b5-9a54-1ab2f3e6bcfc · outbound

This paper cites write newline.

Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations write newline

Reference 2

Resolution: unresolved; no resolver link, observed 2026-08-05T10:57:04.484536Z

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Observation 4bbeacb8-473b-40d8-abda-c34d8c4f998a · outbound

This paper cites In: Bulletin of the American Astronomical Society, p 268.

Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations In: Bulletin of the American Astronomical Society, p 268

Reference 3

Resolution: unresolved; no resolver link, observed 2026-08-05T10:57:04.518123Z

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Observation 27ce4bcb-ac0b-447c-8d28-e40d5af60054 · outbound

This paper cites On the origin of stars with and without planets. Tc trends and clues to Galactic evolution.

Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations On the origin of stars with and without planets. Tc trends and clues to Galactic evolution

Reference 4

Resolution: unresolved; no resolver link, observed 2026-08-05T10:57:04.521450Z

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Observation 178072bc-a3d1-48ed-82c1-07b358bf3daf · outbound

This paper cites The Dispersal of Protoplanetary Disks.

Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations The Dispersal of Protoplanetary Disks

Reference 5

Resolution: unresolved; no resolver link, observed 2026-08-05T10:57:04.525252Z

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Observation 16871188-c148-4a61-a512-3cf6afefdaef · outbound

This paper cites Carbon, oxygen, and iron abundances in disk and halo stars. Implications of 3D non-LTE spectral line formation.

Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations Carbon, oxygen, and iron abundances in disk and halo stars. Implications of 3D non-LTE spectral line formation

Reference 6

Resolution: unresolved; no resolver link, observed 2026-08-05T10:57:04.528776Z

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Observation c15dd44e-a080-4ee7-b5d3-2b1937d525be · outbound

This paper cites The solar carbon, nitrogen, and oxygen abundances from a 3D LTE analysis of molecular lines.

Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations The solar carbon, nitrogen, and oxygen abundances from a 3D LTE analysis of molecular lines

Reference 7

Resolution: unresolved; no resolver link, observed 2026-08-05T10:57:04.532382Z

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Observation 1f958426-f2c8-4282-89da-9056d6623af8 · outbound

This paper cites 3D non-LTE iron abundances in FG-type dwarfs.

Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations 3D non-LTE iron abundances in FG-type dwarfs

Reference 8

Resolution: unresolved; no resolver link, observed 2026-08-05T10:57:04.536085Z

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Observation 49815adb-0d0f-4618-8564-4b0a39076e0d · outbound

This paper cites 43(1):481--530.

Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations 43(1):481--530

Reference 9

Resolution: unresolved; no resolver link, observed 2026-08-05T10:57:04.539508Z

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Observation 93245853-0963-453c-9388-731c7e33d856 · outbound

This paper cites In: Barnes TGIII, Bash FN (eds) Cosmic Abundances as Records of Stellar Evolution and Nucleosynthesis, p 25.

Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations In: Barnes TGIII, Bash FN (eds) Cosmic Abundances as Records of Stellar Evolution and Nucleosynthesis, p 25

Reference 10

Resolution: unresolved; no resolver link, observed 2026-08-05T10:57:04.542331Z

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Observation 82ecb960-9f3f-44fb-af4d-112decb2393e · outbound

This paper cites 47(1):481--522.

Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations 47(1):481--522

Reference 11

Resolution: unresolved; no resolver link, observed 2026-08-05T10:57:04.545270Z

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Observation 22b708f6-aaca-4a14-a684-efbc3a24ee1e · outbound

This paper cites The chemical make-up of the Sun: A 2020 vision.

Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations The chemical make-up of the Sun: A 2020 vision

Reference 12

Resolution: unresolved; no resolver link, observed 2026-08-05T10:57:04.548665Z

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Observation 54431634-971c-465b-9190-97371f8bc96b · outbound

This paper cites HC (2012) RNA Folding and Catalysis Mediated by Iron (II).

Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations HC (2012) RNA Folding and Catalysis Mediated by Iron (II)

Reference 13

Resolution: verified exact; doi, observed 2026-08-05T10:57:05.367676Z

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No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

Observation 79a7f711-7cf1-4bfa-833b-293f66bd1c73 · outbound

This paper cites Exploring the Sun's birth radius and the distribution of planet building blocks in the Milky Way galaxy: A multi-zone Galactic chemical evolution approach.

Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations Exploring the Sun's birth radius and the distribution of planet building blocks in the Milky Way galaxy: A multi-zone Galactic chemical evolution approach

Reference 14

Resolution: unresolved; no resolver link, observed 2026-08-05T10:57:04.554758Z

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Observation 7a443d62-acf9-431a-9714-a431c9154e06 · outbound

This paper cites Structured Distributions of Gas and Solids in Protoplanetary Disks.

Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations Structured Distributions of Gas and Solids in Protoplanetary Disks

Reference 15

Resolution: unresolved; no resolver link, observed 2026-08-05T10:57:04.557602Z

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Observation 7d4ba19f-b269-47b1-b39d-7743d28d1dd0 · outbound

This paper cites Evidence from stable isotopes and Be-10 for solar system formation triggered by a low-mass supernova.

Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations Evidence from stable isotopes and Be-10 for solar system formation triggered by a low-mass supernova

Reference 16

Resolution: unresolved; no resolver link, observed 2026-08-05T10:57:04.560837Z

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Observation 6417e4a5-83a4-4f63-8e1d-812b84ed5802 · outbound

This paper cites Effect of episodic accretion on the structure and the lithium depletion of low-mass stars and planet-hosting stars.

Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations Effect of episodic accretion on the structure and the lithium depletion of low-mass stars and planet-hosting stars

Reference 17

Resolution: unresolved; no resolver link, observed 2026-08-05T10:57:04.563632Z

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Observation 17cae767-d1bf-407b-8504-1b10b0b3f04e · outbound

This paper cites Accurate abundance analysis of late-type stars: advances in atomic physics.

Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations Accurate abundance analysis of late-type stars: advances in atomic physics

Reference 18

Resolution: unresolved; no resolver link, observed 2026-08-05T10:57:04.566563Z

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Observation 9fef0548-2c8e-42a4-9c06-9c41a7dea6a9 · outbound

This paper cites Dust coagulation during the early stages of star formation: molecular cloud collapse and first hydrostatic core evolution.

Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations Dust coagulation during the early stages of star formation: molecular cloud collapse and first hydrostatic core evolution

Reference 19

Resolution: unresolved; no resolver link, observed 2026-08-05T10:57:04.569679Z

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Observation 73e3d2bb-3290-4c7a-89f3-f19273226813 · outbound

This paper cites Lithium depletion in solar-like stars: no planet connection.

Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations Lithium depletion in solar-like stars: no planet connection

Reference 20

Resolution: unresolved; no resolver link, observed 2026-08-05T10:57:04.572797Z

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Observation 41abbe6c-f530-4862-bd59-90e65e7af681 · outbound

This paper cites The Chemical Homogeneity of Sun-like Stars in the Solar Neighborhood.

Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations The Chemical Homogeneity of Sun-like Stars in the Solar Neighborhood

Reference 21

Resolution: unresolved; no resolver link, observed 2026-08-05T10:57:04.576066Z

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Observation 3baaad49-029a-4fbd-8343-2b0cdb3ac2d5 · outbound

This paper cites Planet Engulfment Detections are Rare According to Observations and Stellar Modeling.

Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations Planet Engulfment Detections are Rare According to Observations and Stellar Modeling

Reference 22

Resolution: unresolved; no resolver link, observed 2026-08-05T10:57:04.578901Z

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Observation 2b85bf52-ead7-4ca5-ae39-d2a59b0237bc · outbound

This paper cites In: Niemczura E, Smalley B, Pych W (eds) Determination of Atmospheric Parameters of B.

Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations In: Niemczura E, Smalley B, Pych W (eds) Determination of Atmospheric Parameters of B

Reference 23

Resolution: verified exact; doi, observed 2026-08-05T10:57:05.348052Z

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No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

Observation 0d8d677c-f592-48d4-a70f-c57463a14528 · outbound

This paper cites Observational constraints on the origin of the elements. I. 3D NLTE formation of Mn lines in late-type stars.

Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations Observational constraints on the origin of the elements. I. 3D NLTE formation of Mn lines in late-type stars

Reference 24

Resolution: unresolved; no resolver link, observed 2026-08-05T10:57:04.584266Z

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Observation c477801c-dcf5-4dfc-a612-3f106abae772 · outbound

This paper cites Solar oxygen abundance.

Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations Solar oxygen abundance

Reference 25

Resolution: unresolved; no resolver link, observed 2026-08-05T10:57:04.587013Z

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Observation dd569657-24f0-4e3b-aea5-860246b5410e · outbound

This paper cites The Chemical Composition of the Sun.

Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations The Chemical Composition of the Sun

Reference 26

Resolution: metadata mismatch; local_arxiv, observed 2026-08-05T10:57:05.338440Z

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No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

Observation 67c7c9f7-0511-4bc4-b0bf-f03068b6cca2 · outbound

This paper cites Identifying Young $Kepler$ Planet Host Stars from Keck-HIRES Spectra of Lithium.

Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations Identifying Young $Kepler$ Planet Host Stars from Keck-HIRES Spectra of Lithium

Reference 27

Resolution: unresolved; no resolver link, observed 2026-08-05T10:57:04.592746Z

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Observation 857e8967-6ade-456d-aa0f-fb8615f20895 · outbound

This paper cites The Gaia-ESO Survey: Evidence of atomic diffusion in M67?.

Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations The Gaia-ESO Survey: Evidence of atomic diffusion in M67?

Reference 28

Resolution: unresolved; no resolver link, observed 2026-08-05T10:57:04.595586Z

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Observation 59a255d8-11dc-4d31-933d-bc062f837b29 · outbound

This paper cites The GAPS Programme with HARPS-N at TNG. X. Differential abundances in the XO-2 planet hosting binary.

Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations The GAPS Programme with HARPS-N at TNG. X. Differential abundances in the XO-2 planet hosting binary

Reference 29

Resolution: unresolved; no resolver link, observed 2026-08-05T10:57:04.598334Z

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Observation d790648c-ecaf-40d2-aed6-de4fad53f5a7 · outbound

This paper cites Fingerprints of giant planets in the composition of solar twins.

Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations Fingerprints of giant planets in the composition of solar twins

Reference 30

Resolution: unresolved; no resolver link, observed 2026-08-05T10:57:04.601193Z

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Observation 7fc720b7-3825-424e-a84a-babd748894b1 · outbound

This paper cites Search for giant planets in M67 IV: survey results.

Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations Search for giant planets in M67 IV: survey results

Reference 31

Resolution: unresolved; no resolver link, observed 2026-08-05T10:57:04.604063Z

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Observation cb92d462-3ca2-4f44-a065-e0567aec0434 · outbound

This paper cites In-depth analysis of solar models with high-metallicity abundances and updated opacity tables.

Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations In-depth analysis of solar models with high-metallicity abundances and updated opacity tables

Reference 32

Resolution: unresolved; no resolver link, observed 2026-08-05T10:57:04.607064Z

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Observation 9ea9ec67-014e-4380-9209-95363f170b3d · outbound

This paper cites The photospheric solar oxygen project: I. Abundance analysis of atomic lines and influence of atmospheric models.

Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations The photospheric solar oxygen project: I. Abundance analysis of atomic lines and influence of atmospheric models

Reference 33

Resolution: unresolved; no resolver link, observed 2026-08-05T10:57:04.609891Z

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Observation f5b7dc2c-f3cb-4e2e-87a7-dc5978fbe672 · outbound

This paper cites Solar Chemical Abundances Determined with a CO5BOLD 3D Model Atmosphere.

Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations Solar Chemical Abundances Determined with a CO5BOLD 3D Model Atmosphere

Reference 34

Resolution: unresolved; no resolver link, observed 2026-08-05T10:57:04.612816Z

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Observation 96021705-359a-4214-b2a2-2b0df0cd2dda · outbound

This paper cites The photospheric solar oxygen project: III. Investigation of the centre-to-limb variation of the 630nm [OI]-NiI blend.

Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations The photospheric solar oxygen project: III. Investigation of the centre-to-limb variation of the 630nm [OI]-NiI blend

Reference 35

Resolution: unresolved; no resolver link, observed 2026-08-05T10:57:04.615614Z

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Observation 4f838781-f5d5-40ad-815c-e4ea154ae9cc · outbound

This paper cites Problems of Cosmogeny 7:91.

Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations Problems of Cosmogeny 7:91

Reference 36

Resolution: unresolved; no resolver link, observed 2026-08-05T10:57:04.618955Z

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Observation a65d9920-d9e8-46a7-9c80-3834a8d25e0d · outbound

This paper cites 15(1):121--146.

Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations 15(1):121--146

Reference 37

Resolution: verified exact; doi, observed 2026-08-05T10:57:05.325797Z

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No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

Observation 9f63490b-e19c-48e0-a68e-2ec23310aea0 · outbound

This paper cites The peculiar composition of the Sun is not related to giant planets.

Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations The peculiar composition of the Sun is not related to giant planets

Reference 38

Resolution: unresolved; no resolver link, observed 2026-08-05T10:57:04.624739Z

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Observation f5257970-aa7f-4763-9a77-7ea4116e2139 · outbound

This paper cites A publicly available simulation of an enhanced network region of the Sun.

Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations A publicly available simulation of an enhanced network region of the Sun

Reference 39

Resolution: unresolved; no resolver link, observed 2026-08-05T10:57:04.628183Z

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Observation 509ad2f4-07ab-43f8-913d-b75e6cf922d9 · outbound

This paper cites 94:1--11.

Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations 94:1--11

Reference 40

Resolution: unresolved; no resolver link, observed 2026-08-05T10:57:04.631158Z

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Observation 3ae6ae40-8848-4d80-adce-4789ec3a59b7 · outbound

This paper cites 724(1):92--97.

Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations 724(1):92--97

Reference 41

Resolution: unresolved; no resolver link, observed 2026-08-05T10:57:04.634058Z

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Observation 17418d04-b062-4ebc-adeb-7284f2d11d49 · outbound

This paper cites Solar structure and evolution.

Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations Solar structure and evolution

Reference 42

Resolution: unresolved; no resolver link, observed 2026-08-05T10:57:04.636862Z

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Observation 75a40745-9677-4e66-a91f-55b4cccb4d24 · outbound

This paper cites 121(877):213.

Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations 121(877):213

Reference 43

Resolution: unresolved; no resolver link, observed 2026-08-05T10:57:04.639813Z

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Observation 173b63b0-4908-43db-afd5-35ebca17e575 · outbound

This paper cites ALMA chemical survey of disk-outflow sources in Taurus (ALMA-DOT). IV. Thioformaldehyde (H$_2$CS) in protoplanetary disks: spatial distributions and binding energies.

Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations ALMA chemical survey of disk-outflow sources in Taurus (ALMA-DOT). IV. Thioformaldehyde (H$_2$CS) in protoplanetary disks: spatial distributions and binding energies

Reference 44

Resolution: unresolved; no resolver link, observed 2026-08-05T10:57:04.644139Z

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Observation 7431bd45-da08-4b0d-9a17-eb1f899e64bb · outbound

This paper cites Galactic chemical evolution]{Galactic chemical evolution of the solar neighborhood, solar twins and exoplanet indicators.

Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations Galactic chemical evolution]{Galactic chemical evolution of the solar neighborhood, solar twins and exoplanet indicators

Reference 45

Resolution: unresolved; no resolver link, observed 2026-08-05T10:57:04.647031Z

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Observation 5c1a0653-cd47-4971-b39b-7d1fdaec1b4f · outbound

This paper cites an unresolved cited work.

Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations Unresolved cited work

Reference 46

Resolution: unresolved; no resolver link, observed 2026-08-05T10:57:04.650104Z

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Observation 3a9a5f6d-e02f-4ba1-b8b1-6f9de364b82e · outbound

This paper cites Li depletion in solar analogues with exoplanets: Extending the sample.

Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations Li depletion in solar analogues with exoplanets: Extending the sample

Reference 47

Resolution: unresolved; no resolver link, observed 2026-08-05T10:57:04.652820Z

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Observation 6865b430-c96b-4e1f-b192-e8d12ed9a2d2 · outbound

This paper cites Li abundances in F stars: planets, rotation and galactic evolution.

Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations Li abundances in F stars: planets, rotation and galactic evolution

Reference 48

Resolution: unresolved; no resolver link, observed 2026-08-05T10:57:04.655683Z

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Observation e40fc9cb-f545-47ba-a5a3-a0e7bf20bd37 · outbound

This paper cites The solar photospheric silicon abundance according to CO5BOLD: Investigating line broadening, magnetic fields, and model effects.

Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations The solar photospheric silicon abundance according to CO5BOLD: Investigating line broadening, magnetic fields, and model effects

Reference 49

Resolution: unresolved; no resolver link, observed 2026-08-05T10:57:04.658689Z

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Observation f95e3be2-9969-4b0e-b8d0-8d6c74e52550 · outbound

This paper cites The influence of atomic diffusion on stellar ages and chemical tagging.

Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations The influence of atomic diffusion on stellar ages and chemical tagging

Reference 50

Resolution: unresolved; no resolver link, observed 2026-08-05T10:57:04.662051Z

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Observation 389bee5a-3c8f-43fb-aceb-84f295970309 · outbound

This paper cites Dust Masses, PAH Abundances, and Starlight Intensities in the SINGS Galaxy Sample.

Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations Dust Masses, PAH Abundances, and Starlight Intensities in the SINGS Galaxy Sample

Reference 51

Resolution: unresolved; no resolver link, observed 2026-08-05T10:57:04.665170Z

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Observation 584ab1d2-1e69-48c3-bcda-3cb721fb8f94 · outbound

This paper cites Stellar Multiplicity.

Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations Stellar Multiplicity

Reference 52

Resolution: unresolved; no resolver link, observed 2026-08-05T10:57:04.668889Z

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Observation 45d327dd-3414-47fa-9b61-69ae4c42123a · outbound

This paper cites p 39--43, doi:10.1007/3-540-54752-5_186.

Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations p 39--43, doi:10.1007/3-540-54752-5_186

Reference 53

Resolution: verified exact; doi, observed 2026-08-05T10:57:05.305042Z

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No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

Observation cda75d8d-beb2-4b3f-b3cc-b996d51bd8fe · outbound

This paper cites Solar Fe abundance and magnetic fields - Towards a consistent reference metallicity.

Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations Solar Fe abundance and magnetic fields - Towards a consistent reference metallicity

Reference 54

Resolution: unresolved; no resolver link, observed 2026-08-05T10:57:04.674637Z

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Observation 2c012eff-0023-45fd-8f9a-5b5512afa0c9 · outbound

This paper cites Hints for a Turnover at the Snow Line in the Giant Planet Occurrence Rate.

Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations Hints for a Turnover at the Snow Line in the Giant Planet Occurrence Rate

Reference 55

Resolution: unresolved; no resolver link, observed 2026-08-05T10:57:04.677842Z

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Observation 1137814b-0beb-4575-898c-7862a51aa364 · outbound

This paper cites In: Gomes N, Ascenso J (eds) 24th Portuguese National Astronomy and Astrophysics Meeting, p 51.

Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations In: Gomes N, Ascenso J (eds) 24th Portuguese National Astronomy and Astrophysics Meeting, p 51

Reference 56

Resolution: unresolved; no resolver link, observed 2026-08-05T10:57:04.680875Z

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Observation 6eb2b646-28bb-4922-989f-dae2f6d517bd · outbound

This paper cites Astronomische Nachrichten 323:213--219.

Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations Astronomische Nachrichten 323:213--219

Reference 57

Resolution: unresolved; no resolver link, observed 2026-08-05T10:57:04.683663Z

Source-reported events for the cited work

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Observation 0a40e9ff-342b-4095-86be-a580dda69c66 · outbound

This paper cites 922(2):129.

Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations 922(2):129

Reference 58

Resolution: unresolved; no resolver link, observed 2026-08-05T10:57:04.686498Z

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Observation 84521fda-b9dc-4663-87c0-5526e22f52fc · outbound

This paper cites Cell 168(6).

Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations Cell 168(6)

Reference 59

Resolution: unresolved; no resolver link, observed 2026-08-05T10:57:04.689316Z

Source-reported events for the cited work

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Observation 0d47bfe4-2667-47e2-aa60-4084229885d1 · outbound

This paper cites 285(2):403--412.

Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations 285(2):403--412

Reference 60

Resolution: unresolved; no resolver link, observed 2026-08-05T10:57:04.692297Z

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Observation b7c0f852-ed7e-436d-b314-6f63cc38a736 · outbound

This paper cites The Chemical Compositions of Stars with Planets: A Review.

Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations The Chemical Compositions of Stars with Planets: A Review

Reference 61

Resolution: unresolved; no resolver link, observed 2026-08-05T10:57:04.695058Z

Source-reported events for the cited work

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Observation aefc9494-45b5-4306-831d-4dd89f176689 · outbound

This paper cites Solar System chemical abundances corrected for systematics.

Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations Solar System chemical abundances corrected for systematics

Reference 62

Resolution: unresolved; no resolver link, observed 2026-08-05T10:57:04.698258Z

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Observation a8dd385f-608f-415d-b9a1-9e7b23dec4b2 · outbound

This paper cites In: Holt SS, Sonneborn G (eds) Cosmic Abundances, p 117.

Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations In: Holt SS, Sonneborn G (eds) Cosmic Abundances, p 117

Reference 63

Resolution: unresolved; no resolver link, observed 2026-08-05T10:57:04.701103Z

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Observation fe64d4b9-f0d7-48c6-832c-d97ecb5d4234 · outbound

This paper cites doi:10.1023/A:1005164331058.

Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations doi:10.1023/A:1005164331058

Reference 64

Resolution: verified exact; doi, observed 2026-08-05T10:57:05.276394Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

Observation 671fead2-9bff-4140-b002-e94a03e76de6 · outbound

This paper cites Dust cleansing of star-forming gas I: Did radiation from bright stars affect the chemical composition of the Sun and of M67?.

Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations Dust cleansing of star-forming gas I: Did radiation from bright stars affect the chemical composition of the Sun and of M67?

Reference 65

Resolution: unresolved; no resolver link, observed 2026-08-05T10:57:04.706846Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 8d56708a-cb25-40a1-a999-e733dbf74be2 · outbound

This paper cites Dust cleansing of star-forming gas: II. Did late accretion flows change the chemical composition of the solar atmosphere?.

Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations Dust cleansing of star-forming gas: II. Did late accretion flows change the chemical composition of the solar atmosphere?

Reference 66

Resolution: unresolved; no resolver link, observed 2026-08-05T10:57:04.709772Z

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Observation 623fdcb5-9807-4a41-8f11-36f36f82de3d · outbound

This paper cites 328(1-2):185--191.

Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations 328(1-2):185--191

Reference 67

Resolution: unresolved; no resolver link, observed 2026-08-05T10:57:04.712725Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation df809858-d31a-4ab1-8da9-3a7e24c32664 · outbound

This paper cites Condensation of Dust Particles.

Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations Condensation of Dust Particles

Reference 68

Resolution: verified exact; doi, observed 2026-08-05T10:57:05.260212Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

Observation 391d5044-05dc-4f8b-b75b-bf27c331373b · outbound

This paper cites The abundance pattern of the lambda Bootis stars.

Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations The abundance pattern of the lambda Bootis stars

Reference 69

Resolution: unresolved; no resolver link, observed 2026-08-05T10:57:04.718691Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 9cf6d7e0-a194-4b96-bd66-f8f626c605a2 · outbound

This paper cites The accretion/diffusion theory for lambda Bootis stars in the light of spectroscopic data.

Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations The accretion/diffusion theory for lambda Bootis stars in the light of spectroscopic data

Reference 70

Resolution: unresolved; no resolver link, observed 2026-08-05T10:57:04.721590Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation bfee1ac9-1463-4a2c-b6ff-3dbc7b8657f3 · outbound

This paper cites Stellar Wind Yields of Very Massive Stars.

Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations Stellar Wind Yields of Very Massive Stars

Reference 71

Resolution: unresolved; no resolver link, observed 2026-08-05T10:57:04.724433Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d63fb063-283b-4f57-8812-4a0431db9bf5 · outbound

This paper cites In: Dworetsky MM, Castelli F, Faraggiana R (eds) IAU Colloq.

Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations In: Dworetsky MM, Castelli F, Faraggiana R (eds) IAU Colloq

Reference 72

Resolution: unresolved; no resolver link, observed 2026-08-05T10:57:04.727306Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 5dba7fa7-4f1d-4435-a647-791b28640acd · outbound

This paper cites The Fundamentally Different Dynamics of Dust and Gas in Molecular Clouds.

Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations The Fundamentally Different Dynamics of Dust and Gas in Molecular Clouds

Reference 73

Resolution: unresolved; no resolver link, observed 2026-08-05T10:57:04.730098Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 865304a9-1621-445d-8d6e-f46aff615d66 · outbound

This paper cites Earth and Planetary Science Letters 487:9--20.

Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations Earth and Planetary Science Letters 487:9--20

Reference 74

Resolution: verified exact; doi, observed 2026-08-05T10:57:05.250824Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

Observation 9eaedb19-e94a-42cd-879a-656ce52634c4 · outbound

This paper cites How does accretion of planet-forming disks influence stellar abundances?.

Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations How does accretion of planet-forming disks influence stellar abundances?

Reference 75

Resolution: unresolved; no resolver link, observed 2026-08-05T10:57:04.735744Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation caac975e-54b0-4d87-b37f-8f389f91b2e0 · outbound

This paper cites 363(1):293--314.

Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations 363(1):293--314

Reference 76

Resolution: unresolved; no resolver link, observed 2026-08-05T10:57:04.739619Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 2ec82342-fea9-4a89-b9d8-9300c2eb34ea · outbound

This paper cites Enhanced lithium depletion in Sun-like stars with orbiting planets.

Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations Enhanced lithium depletion in Sun-like stars with orbiting planets

Reference 77

Resolution: unresolved; no resolver link, observed 2026-08-05T10:57:04.742460Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a1ff75db-5ed4-4db1-9fd0-58e81072761e · outbound

This paper cites Gas giant planets as dynamical barriers to inward-migrating super-Earths.

Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations Gas giant planets as dynamical barriers to inward-migrating super-Earths

Reference 78

Resolution: unresolved; no resolver link, observed 2026-08-05T10:57:04.745866Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation af20abcc-032d-4b44-b35f-c4900789fc6c · outbound

This paper cites Breaking the Chains: Hot Super-Earth systems from migration and disruption of compact resonant chains.

Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations Breaking the Chains: Hot Super-Earth systems from migration and disruption of compact resonant chains

Reference 79

Resolution: unresolved; no resolver link, observed 2026-08-05T10:57:04.749153Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation bd18b216-ddbb-4f39-9255-4f1005caf2c9 · outbound

This paper cites Gaia FGK benchmark stars: abundances of alpha and iron-peak elements.

Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations Gaia FGK benchmark stars: abundances of alpha and iron-peak elements

Reference 80

Resolution: unresolved; no resolver link, observed 2026-08-05T10:57:04.752237Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f51a9b59-0cb6-484c-ae85-888d4440c019 · outbound

This paper cites Accuracy and precision of industrial stellar abundances.

Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations Accuracy and precision of industrial stellar abundances

Reference 81

Resolution: unresolved; no resolver link, observed 2026-08-05T10:57:04.755542Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation aa43aea1-57b4-4f96-b7fb-3d2f64b87fda · outbound

This paper cites In: American Astronomical Society Meeting Abstracts, p 340.04D.

Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations In: American Astronomical Society Meeting Abstracts, p 340.04D

Reference 82

Resolution: unresolved; no resolver link, observed 2026-08-05T10:57:04.758694Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 1e60c769-7c33-4d94-8dfc-56ac540bd007 · outbound

This paper cites Dust in the Wind: Composition and Kinematics of Galaxy Outflows at the Peak Epoch of Star Formation.

Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations Dust in the Wind: Composition and Kinematics of Galaxy Outflows at the Peak Epoch of Star Formation

Reference 83

Resolution: unresolved; no resolver link, observed 2026-08-05T10:57:04.762790Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 42a6e45b-7400-44d7-b4d4-be7d8a51c3f5 · outbound

This paper cites Lambda Boo Abundance Patterns: Accretion from Orbiting Sources.

Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations Lambda Boo Abundance Patterns: Accretion from Orbiting Sources

Reference 84

Resolution: unresolved; no resolver link, observed 2026-08-05T10:57:04.766560Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e554936f-eea0-43dd-a27b-3aa6af2cb088 · outbound

This paper cites Meteoritics & Planetary Science 59(12):3193--3214.

Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations Meteoritics & Planetary Science 59(12):3193--3214

Reference 85

Resolution: verified exact; doi, observed 2026-08-05T10:57:05.241055Z

Source-reported events for the cited work

correction dated 2025-11-11. Source: crossref record 10.1111/maps.70059->10.1111/maps.14272:correction, observed 2026-07-11T02:55:43.045809+00:00. This notice travels one citation hop only.

Observation 07c34379-ad89-493d-bf11-d49651443cc1 · outbound

This paper cites 335(2):L45--L49.

Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations 335(2):L45--L49

Reference 86

Resolution: unresolved; no resolver link, observed 2026-08-05T10:57:04.772273Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a5c608cc-6560-47b3-abe6-25dca3e76880 · outbound

This paper cites 91(1-2):175--180.

Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations 91(1-2):175--180

Reference 87

Resolution: unresolved; no resolver link, observed 2026-08-05T10:57:04.775042Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 2fcd3489-9c7c-4303-8289-ad2308b07e54 · outbound

This paper cites Is the solar spectrum latitude dependent? An investigation with SST/TRIPPEL.

Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations Is the solar spectrum latitude dependent? An investigation with SST/TRIPPEL

Reference 88

Resolution: unresolved; no resolver link, observed 2026-08-05T10:57:04.778338Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 548b6fe2-9ae4-401f-be39-1e51c3976c39 · outbound

This paper cites Atomic Diffusion and Mixing in Old Stars I. VLT/FLAMES-UVES Observations of Stars in NGC 6397.

Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations Atomic Diffusion and Mixing in Old Stars I. VLT/FLAMES-UVES Observations of Stars in NGC 6397

Reference 89

Resolution: unresolved; no resolver link, observed 2026-08-05T10:57:04.781406Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 971d826c-885a-4c35-b1cd-c5ea3b8be6ca · outbound

This paper cites doi:10.1002/chem.201801847.

Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations doi:10.1002/chem.201801847

Reference 90

Resolution: verified exact; doi, observed 2026-08-05T10:57:05.231157Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

Observation ab4d9009-27d8-4d6c-9c59-d881c7794c53 · outbound

This paper cites Evolution of the Milky Way with radial motions of stars and gas I. The solar neighborhood and the thin and thick disk.

Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations Evolution of the Milky Way with radial motions of stars and gas I. The solar neighborhood and the thin and thick disk

Reference 91

Resolution: unresolved; no resolver link, observed 2026-08-05T10:57:04.787515Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 9d0ba377-0239-4012-aa6b-059675bffa2c · outbound

This paper cites Zoom-Simulations of Protoplanetary Disks starting from GMC scales.

Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations Zoom-Simulations of Protoplanetary Disks starting from GMC scales

Reference 92

Resolution: unresolved; no resolver link, observed 2026-08-05T10:57:04.791244Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation bedc2a06-0ae7-4f81-b0a2-a6f3ae2234e3 · outbound

This paper cites Revisiting the pre-main-sequence evolution of stars I. Importance of accretion efficiency and deuterium abundance.

Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations Revisiting the pre-main-sequence evolution of stars I. Importance of accretion efficiency and deuterium abundance

Reference 93

Resolution: unresolved; no resolver link, observed 2026-08-05T10:57:04.794516Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 39195dde-5d8f-418b-be8d-ed8a1d1702e1 · outbound

This paper cites Revisiting the pre-main-sequence evolution of stars II. Consequences of planet formation on stellar surface composition.

Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations Revisiting the pre-main-sequence evolution of stars II. Consequences of planet formation on stellar surface composition

Reference 94

Resolution: unresolved; no resolver link, observed 2026-08-05T10:57:04.797435Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 94dc4cc7-38b2-44d9-999b-f7db0c145a47 · outbound

This paper cites Probing the strength of radial migration via churning by using metal-rich red giant stars from APOGEE.

Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations Probing the strength of radial migration via churning by using metal-rich red giant stars from APOGEE

Reference 95

Resolution: unresolved; no resolver link, observed 2026-08-05T10:57:04.800748Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c5785cfb-6b2c-4f7b-9da3-e701f08d1543 · outbound

This paper cites Super-Earths and Earth-like Exoplanets.

Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations Super-Earths and Earth-like Exoplanets

Reference 96

Resolution: unresolved; no resolver link, observed 2026-08-05T10:57:04.803883Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 5219234d-cb4d-4e32-8d2e-b41df4150ee1 · outbound

This paper cites 3D non-LTE abundance analyses of late-type stars.

Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations 3D non-LTE abundance analyses of late-type stars

Reference 97

Resolution: unresolved; no resolver link, observed 2026-08-05T10:57:04.806913Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 85aea0b7-61d1-45bd-8ad4-a008b4232c37 · outbound

This paper cites The chemical compositions of solar twins in the open cluster M67.

Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations The chemical compositions of solar twins in the open cluster M67

Reference 98

Resolution: unresolved; no resolver link, observed 2026-08-05T10:57:04.809974Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 147f2a17-8959-448d-8b0c-15ace6691018 · outbound

This paper cites The Hyades open cluster is chemically inhomogeneous.

Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations The Hyades open cluster is chemically inhomogeneous

Reference 99

Resolution: unresolved; no resolver link, observed 2026-08-05T10:57:04.812927Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ace9b7c4-a5fa-4637-8b8f-00397fd32dda · outbound

This paper cites Chemical (in)homogeneity and atomic diffusion in the open cluster M67.

Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations Chemical (in)homogeneity and atomic diffusion in the open cluster M67

Reference 100

Resolution: unresolved; no resolver link, observed 2026-08-05T10:57:04.816136Z

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Unavailable: canonical work link unavailable.

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