The complex stellar system M 22: confirming abundance variations with high precision differential measurements | Paper Citation Record

Observation e815d53b-a295-4e9b-9c3c-6dc176e7fe62 · outbound

This paper cites Mg isotopic ratios in giant stars of the globular cluster NGC 6752.

The complex stellar system M 22: confirming abundance variations with high precision differential measurements Mg isotopic ratios in giant stars of the globular cluster NGC 6752

Reference 1

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Observation 12986593-a5a8-4bc0-889d-01cb80b41c04 · outbound

This paper cites Heavy elements in Globular Clusters: the role of AGB stars.

The complex stellar system M 22: confirming abundance variations with high precision differential measurements Heavy elements in Globular Clusters: the role of AGB stars

Reference 2

Resolution: unresolved; no resolver link, observed 2026-08-02T02:58:15.113418Z

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Observation 5ae631a5-ec93-419c-80f3-e23d36a8363d · outbound

This paper cites The s-Process Enrichment of the Globular Clusters M4 and M22.

The complex stellar system M 22: confirming abundance variations with high precision differential measurements The s-Process Enrichment of the Globular Clusters M4 and M22

Reference 3

Resolution: unresolved; no resolver link, observed 2026-08-02T02:58:15.192685Z

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Observation ac4c28d2-1f47-4c52-877f-bca4545b2d58 · outbound

This paper cites High Precision Differential Abundance Measurements in Globular Clusters: Chemical Inhomogeneities in NGC 6752.

The complex stellar system M 22: confirming abundance variations with high precision differential measurements High Precision Differential Abundance Measurements in Globular Clusters: Chemical Inhomogeneities in NGC 6752

Reference 5

Resolution: unresolved; no resolver link, observed 2026-08-02T02:58:15.417690Z

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Observation d0d6660f-8887-4a38-a60b-bc73017d2e66 · outbound

This paper cites A double stellar generation in the Globular Cluster NGC6656 (M 22). Two stellar groups with different iron and s-process element abundance.

The complex stellar system M 22: confirming abundance variations with high precision differential measurements A double stellar generation in the Globular Cluster NGC6656 (M 22). Two stellar groups with different iron and s-process element abundance

Reference 6

Resolution: unresolved; no resolver link, observed 2026-08-02T02:58:15.491180Z

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Observation 268f31b8-a369-4236-9a05-f99515f04482 · outbound

This paper cites The two metallicity groups of the globular cluster M22: a chemical perspective.

The complex stellar system M 22: confirming abundance variations with high precision differential measurements The two metallicity groups of the globular cluster M22: a chemical perspective

Reference 7

Resolution: unresolved; no resolver link, observed 2026-08-02T02:58:15.585044Z

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Observation 29986b97-f93b-45d8-9e56-69fefad9b953 · outbound

This paper cites arXiv e-prints , keywords =.

The complex stellar system M 22: confirming abundance variations with high precision differential measurements arXiv e-prints , keywords =

Reference 8

Resolution: unresolved; no resolver link, observed 2026-08-02T02:58:15.692263Z

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Observation 069d0f13-e65f-4700-9ad2-6f28534b1261 · outbound

This paper cites Metallicity Fluctuation Statistics in the Interstellar Medium and Young Stars. I. Variance and Correlation.

The complex stellar system M 22: confirming abundance variations with high precision differential measurements Metallicity Fluctuation Statistics in the Interstellar Medium and Young Stars. I. Variance and Correlation

Reference 9

Resolution: unresolved; no resolver link, observed 2026-08-02T02:58:15.831545Z

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Observation 0fa7a1a2-fd1f-4f14-8cb4-3e1fba025d7b · outbound

This paper cites SLUG IV: A Novel Forward-Modelling Method to Derive the Demographics of Star Clusters.

The complex stellar system M 22: confirming abundance variations with high precision differential measurements SLUG IV: A Novel Forward-Modelling Method to Derive the Demographics of Star Clusters

Reference 10

Resolution: unresolved; no resolver link, observed 2026-08-02T02:58:15.833901Z

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Observation f5750ea8-243a-42dc-bc14-85d7fb7424d0 · outbound

This paper cites SLUG -- Stochastically Lighting Up Galaxies. III: A Suite of Tools for Simulated Photometry, Spectroscopy, and Bayesian Inference with Stochastic Stellar Populations.

The complex stellar system M 22: confirming abundance variations with high precision differential measurements SLUG -- Stochastically Lighting Up Galaxies. III: A Suite of Tools for Simulated Photometry, Spectroscopy, and Bayesian Inference with Stochastic Stellar Populations

Reference 11

Resolution: unresolved; no resolver link, observed 2026-08-02T02:58:15.835871Z

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Observation 1cfab7cd-1f7a-455d-a4e1-eb5e374e4248 · outbound

This paper cites SLUG - Stochastically Lighting Up Galaxies. II: Quantifying the Effects of Stochasticity on Star Formation Rate Indicators.

The complex stellar system M 22: confirming abundance variations with high precision differential measurements SLUG - Stochastically Lighting Up Galaxies. II: Quantifying the Effects of Stochasticity on Star Formation Rate Indicators

Reference 12

Resolution: unresolved; no resolver link, observed 2026-08-02T02:58:15.838592Z

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Observation c2353823-a49f-4092-83f2-53433858f73e · outbound

This paper cites SLUG - Stochastically Lighting Up Galaxies I: Methods and Validating Tests.

The complex stellar system M 22: confirming abundance variations with high precision differential measurements SLUG - Stochastically Lighting Up Galaxies I: Methods and Validating Tests

Reference 13

Resolution: unresolved; no resolver link, observed 2026-08-02T02:58:15.840674Z

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Observation 5c1dcc44-6e3b-4ca4-89e3-96610d3c14d3 · outbound

This paper cites Characterizing the Heavy Elements in Globular Cluster M22 and an Empirical s-process Abundance Distribution Derived from the Two Stellar Groups.

The complex stellar system M 22: confirming abundance variations with high precision differential measurements Characterizing the Heavy Elements in Globular Cluster M22 and an Empirical s-process Abundance Distribution Derived from the Two Stellar Groups

Reference 14

Resolution: unresolved; no resolver link, observed 2026-08-02T02:58:15.842761Z

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Observation a6c2e133-c3bd-4323-a9cf-bb60c2279479 · outbound

This paper cites , keywords =.

The complex stellar system M 22: confirming abundance variations with high precision differential measurements , keywords =

Reference 15

Resolution: verified exact; doi, observed 2026-08-02T02:59:26.466704Z

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Observation 3b91cbe5-02d0-4b68-be6f-a233b572215b · outbound

This paper cites CNO and F abundances in the globular cluster M22 (NGC 6656).

The complex stellar system M 22: confirming abundance variations with high precision differential measurements CNO and F abundances in the globular cluster M22 (NGC 6656)

Reference 16

Resolution: unresolved; no resolver link, observed 2026-08-02T02:58:15.847771Z

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Observation 14456325-0086-41ea-8db5-8a465b478510 · outbound

This paper cites Core-Collapse Supernovae from 9 to 120 Solar Masses Based on Neutrino-powered Explosions.

The complex stellar system M 22: confirming abundance variations with high precision differential measurements Core-Collapse Supernovae from 9 to 120 Solar Masses Based on Neutrino-powered Explosions

Reference 17

Resolution: unresolved; no resolver link, observed 2026-08-02T02:58:15.850317Z

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Observation d09e4698-d115-45b5-839b-baad754135d5 · outbound

This paper cites Super and Massive AGB Stars: II - Nucleosynthesis and Yields - Z=0.02, 0.008 and 0.004.

The complex stellar system M 22: confirming abundance variations with high precision differential measurements Super and Massive AGB Stars: II - Nucleosynthesis and Yields - Z=0.02, 0.008 and 0.004

Reference 18

Resolution: unresolved; no resolver link, observed 2026-08-02T02:58:15.852436Z

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Observation ea02cbdc-b4d9-4036-91e6-acb9bcaec373 · outbound

This paper cites Stellar yields from metal-rich asymptotic giant branch models.

The complex stellar system M 22: confirming abundance variations with high precision differential measurements Stellar yields from metal-rich asymptotic giant branch models

Reference 19

Resolution: unresolved; no resolver link, observed 2026-08-02T02:58:15.854359Z

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Observation be40d974-0240-4b6d-a1f3-e16dd168c8ce · outbound

This paper cites The Impact of Starbursts on Element Abundance Ratios.

The complex stellar system M 22: confirming abundance variations with high precision differential measurements The Impact of Starbursts on Element Abundance Ratios

Reference 20

Resolution: unresolved; no resolver link, observed 2026-08-02T02:58:15.857094Z

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Observation 9be9c024-13fa-4f75-b61f-7336af784c41 · outbound

This paper cites arXiv e-prints , keywords =.

The complex stellar system M 22: confirming abundance variations with high precision differential measurements arXiv e-prints , keywords =

Reference 21

Resolution: unresolved; no resolver link, observed 2026-08-02T02:58:15.859804Z

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Observation 03a7e50d-c6be-4619-883f-ae827964d301 · outbound

This paper cites The Similarity of Abundance Ratio Trends and Nucleosynthetic Patterns in the Milky Way Disk and Bulge.

The complex stellar system M 22: confirming abundance variations with high precision differential measurements The Similarity of Abundance Ratio Trends and Nucleosynthetic Patterns in the Milky Way Disk and Bulge

Reference 22

Resolution: unresolved; no resolver link, observed 2026-08-02T02:58:15.862459Z

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Observation 1d007fda-4582-4342-b570-24a35aa10587 · outbound

This paper cites Abundance ratios in GALAH DR2 and their implications for nucleosynthesis.

The complex stellar system M 22: confirming abundance variations with high precision differential measurements Abundance ratios in GALAH DR2 and their implications for nucleosynthesis

Reference 23

Resolution: unresolved; no resolver link, observed 2026-08-02T02:58:15.864743Z

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Observation a5cd76b0-8265-4450-b04e-6dfec0dbef53 · outbound

This paper cites The Origin of Elements from Carbon to Uranium.

The complex stellar system M 22: confirming abundance variations with high precision differential measurements The Origin of Elements from Carbon to Uranium

Reference 24

Resolution: unresolved; no resolver link, observed 2026-08-02T02:58:15.866617Z

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Observation e04c58b4-3b00-4d81-8c37-cfc8f3c6e1f5 · outbound

This paper cites arXiv e-prints , keywords =.

The complex stellar system M 22: confirming abundance variations with high precision differential measurements arXiv e-prints , keywords =

Reference 25

Resolution: unresolved; no resolver link, observed 2026-08-02T02:58:15.868560Z

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Observation 0f4bf8ba-015e-4c56-acce-7d53ad0f1bbd · outbound

This paper cites Chemical Cartography with APOGEE: Multi-element abundance ratios.

The complex stellar system M 22: confirming abundance variations with high precision differential measurements Chemical Cartography with APOGEE: Multi-element abundance ratios

Reference 26

Resolution: unresolved; no resolver link, observed 2026-08-02T02:58:15.870403Z

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Observation e94aa869-d2ee-455a-8014-298a8eeafe8a · outbound

This paper cites arXiv e-prints , keywords =.

The complex stellar system M 22: confirming abundance variations with high precision differential measurements arXiv e-prints , keywords =

Reference 27

Resolution: unresolved; no resolver link, observed 2026-08-02T02:58:15.872374Z

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Observation 72473857-d8a9-4d13-b1f2-a33f00b49460 · outbound

This paper cites Simulating Metal Mixing of Both Common and Rare Enrichment Sources in a Low Mass Dwarf Galaxy.

The complex stellar system M 22: confirming abundance variations with high precision differential measurements Simulating Metal Mixing of Both Common and Rare Enrichment Sources in a Low Mass Dwarf Galaxy

Reference 28

Resolution: unresolved; no resolver link, observed 2026-08-02T02:58:15.874131Z

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Observation c2bd435d-51d9-45aa-902c-54778ddccf28 · outbound

This paper cites Mixing of metals during star cluster formation: statistics and implications for chemical tagging.

The complex stellar system M 22: confirming abundance variations with high precision differential measurements Mixing of metals during star cluster formation: statistics and implications for chemical tagging

Reference 29

Resolution: unresolved; no resolver link, observed 2026-08-02T02:58:15.876264Z

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Observation c11ba771-4fba-438c-a6a8-7ba0a33bde23 · outbound

This paper cites LYRA I: Simulating the multi-phase ISM of a dwarf galaxy with variable energy supernovae from individual stars.

The complex stellar system M 22: confirming abundance variations with high precision differential measurements LYRA I: Simulating the multi-phase ISM of a dwarf galaxy with variable energy supernovae from individual stars

Reference 30

Resolution: unresolved; no resolver link, observed 2026-08-02T02:58:15.878275Z

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Observation 7cdbabaa-315d-4097-9f1f-0edcbebcbf9c · outbound

This paper cites Dust-regulated galaxy formation and evolution:A new chemodynamical model with live dust particles.

The complex stellar system M 22: confirming abundance variations with high precision differential measurements Dust-regulated galaxy formation and evolution:A new chemodynamical model with live dust particles

Reference 31

Resolution: unresolved; no resolver link, observed 2026-08-02T02:58:15.880472Z

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Observation 68dfef8f-7d42-4fc7-bc2b-4077e982c9c4 · outbound

This paper cites , keywords =.

The complex stellar system M 22: confirming abundance variations with high precision differential measurements , keywords =

Reference 32

Resolution: unresolved; no resolver link, observed 2026-08-02T02:58:15.882425Z

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Observation 088db703-f182-4266-9e1e-0afee773e70b · outbound

This paper cites Detection of metallicity correlations in 100 nearby galaxies.

The complex stellar system M 22: confirming abundance variations with high precision differential measurements Detection of metallicity correlations in 100 nearby galaxies

Reference 33

Resolution: unresolved; no resolver link, observed 2026-08-02T02:58:15.884172Z

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Observation 8def89a9-9fec-438c-a82d-3a307d06d5b2 · outbound

This paper cites Measuring the mixing scale of the ISM within nearby spiral galaxies.

The complex stellar system M 22: confirming abundance variations with high precision differential measurements Measuring the mixing scale of the ISM within nearby spiral galaxies

Reference 34

Resolution: unresolved; no resolver link, observed 2026-08-02T02:58:15.886266Z

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Observation 1b0e6c54-6c65-4417-af5a-41c4a3d3ff9f · outbound

This paper cites Mapping metallicity variations across nearby galaxy disks.

The complex stellar system M 22: confirming abundance variations with high precision differential measurements Mapping metallicity variations across nearby galaxy disks

Reference 35

Resolution: unresolved; no resolver link, observed 2026-08-02T02:58:15.888212Z

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Observation 127912b1-0ab8-49e8-8f1f-0b22760e2f30 · outbound

This paper cites 3-D gas-phase elemental abundances across the formation histories of Milky Way-mass galaxies in the FIRE simulations: initial conditions for chemical tagging.

The complex stellar system M 22: confirming abundance variations with high precision differential measurements 3-D gas-phase elemental abundances across the formation histories of Milky Way-mass galaxies in the FIRE simulations: initial conditions for chemical tagging

Reference 36

Resolution: unresolved; no resolver link, observed 2026-08-02T02:58:15.890255Z

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Observation 18447e29-eb00-4ed5-801f-64bd7b7ae7a8 · outbound

This paper cites Numerical convergence of hydrodynamical simulations of galaxy formation: the abundance and internal structure of galaxies and their cold dark matter haloes.

The complex stellar system M 22: confirming abundance variations with high precision differential measurements Numerical convergence of hydrodynamical simulations of galaxy formation: the abundance and internal structure of galaxies and their cold dark matter haloes

Reference 37

Resolution: unresolved; no resolver link, observed 2026-08-02T02:58:15.892365Z

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Observation a485c2ab-45f5-4ad7-bae9-e5a5902f9cb0 · outbound

This paper cites The Solar Twin Planet Search. I. Fundamental parameters of the stellar sample.

The complex stellar system M 22: confirming abundance variations with high precision differential measurements The Solar Twin Planet Search. I. Fundamental parameters of the stellar sample

Reference 38

Resolution: unresolved; no resolver link, observed 2026-08-02T02:58:15.894407Z

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Observation 9bad002f-13b6-46ee-973d-a1061003ad65 · outbound

This paper cites , year = 1973, month = sep, volume =.

The complex stellar system M 22: confirming abundance variations with high precision differential measurements , year = 1973, month = sep, volume =

Reference 39

Resolution: unresolved; no resolver link, observed 2026-08-02T02:58:15.896354Z

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Observation ef54442b-e4fd-4026-891f-54fc534ffedb · outbound

This paper cites The chemical composition of red giants in 47 Tucanae. II. Magnesium isotopes and pollution scenarios.

The complex stellar system M 22: confirming abundance variations with high precision differential measurements The chemical composition of red giants in 47 Tucanae. II. Magnesium isotopes and pollution scenarios

Reference 40

Resolution: unresolved; no resolver link, observed 2026-08-02T02:58:15.898403Z

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Observation 322004b4-ca66-47fd-b528-473df51dc552 · outbound

This paper cites Magnesium Isotope Ratios in omega Centauri Red Giants.

The complex stellar system M 22: confirming abundance variations with high precision differential measurements Magnesium Isotope Ratios in omega Centauri Red Giants

Reference 41

Resolution: unresolved; no resolver link, observed 2026-08-02T02:58:15.900306Z

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Observation 0621fda5-ce73-4c08-9dc1-2a2caa46f40e · outbound

This paper cites DAOSPEC: an automatic code for measuring equivalent widths in high-resolution stellar spectra.

The complex stellar system M 22: confirming abundance variations with high precision differential measurements DAOSPEC: an automatic code for measuring equivalent widths in high-resolution stellar spectra

Reference 42

Resolution: unresolved; no resolver link, observed 2026-08-02T02:58:15.902271Z

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Observation 039b6c4b-9787-4d7d-988a-e9a99b477e69 · outbound

This paper cites Magnesium isotope ratios in Hyades stars.

The complex stellar system M 22: confirming abundance variations with high precision differential measurements Magnesium isotope ratios in Hyades stars

Reference 43

Resolution: unresolved; no resolver link, observed 2026-08-02T02:58:15.904185Z

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Observation 19088572-b68e-42b9-90ca-196ff9a35f20 · outbound

This paper cites an unresolved cited work.

The complex stellar system M 22: confirming abundance variations with high precision differential measurements Unresolved cited work

Reference 44

Resolution: unresolved; no resolver link, observed 2026-08-02T02:58:15.907009Z

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Observation 35f8d063-b0e3-4f50-ae53-0b9e736c1a45 · outbound

This paper cites Gaia and Hubble unveil the kinematics of stellar populations in the Type II globular clusters {\omega} Centauri and M 22.

The complex stellar system M 22: confirming abundance variations with high precision differential measurements Gaia and Hubble unveil the kinematics of stellar populations in the Type II globular clusters {\omega} Centauri and M 22

Reference 45

Resolution: unresolved; no resolver link, observed 2026-08-02T02:58:15.909044Z

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Observation 1273d821-d28e-487b-98b2-b669cf160f58 · outbound

This paper cites M22: A [Fe/H] Abundance Range Revealed.

The complex stellar system M 22: confirming abundance variations with high precision differential measurements M22: A [Fe/H] Abundance Range Revealed

Reference 46

Resolution: unresolved; no resolver link, observed 2026-08-02T02:58:15.911217Z

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Observation 83b1b5a4-e242-4be0-8c67-0877439339a1 · outbound

This paper cites Star Clusters , year = 1980, editor =.

The complex stellar system M 22: confirming abundance variations with high precision differential measurements Star Clusters , year = 1980, editor =

Reference 47

Resolution: unresolved; no resolver link, observed 2026-08-02T02:58:15.913262Z

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Observation a1358440-5304-41ea-8d33-456607092999 · outbound

This paper cites , keywords =.

The complex stellar system M 22: confirming abundance variations with high precision differential measurements , keywords =

Reference 48

Resolution: verified exact; doi, observed 2026-08-02T02:59:26.274078Z

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 a5058098-6564-4e9e-b413-5de0067d45d9 · outbound

This paper cites , year = 1977, month = apr, volume =.

The complex stellar system M 22: confirming abundance variations with high precision differential measurements , year = 1977, month = apr, volume =

Reference 49

Resolution: verified exact; doi, observed 2026-08-02T02:59:26.066136Z

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 f498149b-971c-40d3-968f-55ad8805f475 · outbound

This paper cites , keywords =.

The complex stellar system M 22: confirming abundance variations with high precision differential measurements , keywords =

Reference 50

Resolution: verified exact; doi, observed 2026-08-02T02:59:25.803799Z

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 2d9fa60c-0ed1-4015-997e-dce70fa460c1 · outbound

This paper cites , year = 1975, month = oct, volume =.

The complex stellar system M 22: confirming abundance variations with high precision differential measurements , year = 1975, month = oct, volume =

Reference 51

Resolution: unresolved; no resolver link, observed 2026-08-02T02:58:15.921599Z

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Observation 06ef87b6-9c60-476f-afe0-35bd40a23f80 · outbound

This paper cites , year = 1975, month = oct, volume =.

The complex stellar system M 22: confirming abundance variations with high precision differential measurements , year = 1975, month = oct, volume =

Reference 52

Resolution: verified exact; doi, observed 2026-08-02T02:59:25.534337Z

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 ede466dc-8e62-4d19-b4c3-a505660e1b93 · outbound

This paper cites The anomalous giant branch of omega Centauri.

The complex stellar system M 22: confirming abundance variations with high precision differential measurements The anomalous giant branch of omega Centauri

Reference 53

Resolution: verified exact; doi, observed 2026-08-02T02:59:25.297209Z

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 2b6f969a-9d3c-4e5b-bd17-c0deafe33e9b · outbound

This paper cites , keywords =.

The complex stellar system M 22: confirming abundance variations with high precision differential measurements , keywords =

Reference 54

Resolution: verified exact; doi, observed 2026-08-02T02:59:25.119647Z

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 dfde9217-a7e7-4abb-a46e-210ef415d13b · outbound

This paper cites , year = 1976, month = oct, volume =.

The complex stellar system M 22: confirming abundance variations with high precision differential measurements , year = 1976, month = oct, volume =

Reference 55

Resolution: verified exact; doi, observed 2026-08-02T02:59:24.868238Z

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 7da8f5e0-1941-4ed2-a9e2-915fe13104d0 · outbound

This paper cites , year = 1976, month = apr, volume =.

The complex stellar system M 22: confirming abundance variations with high precision differential measurements , year = 1976, month = apr, volume =

Reference 56

Resolution: unresolved; no resolver link, observed 2026-08-02T02:58:15.932249Z

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Observation 81135bb5-8033-4235-9ca0-96eb4b7afdd2 · outbound

This paper cites The Observatory , year = 1962, month = oct, volume =.

The complex stellar system M 22: confirming abundance variations with high precision differential measurements The Observatory , year = 1962, month = oct, volume =

Reference 57

Resolution: unresolved; no resolver link, observed 2026-08-02T02:58:15.933921Z

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Observation 87e48fdd-4ce4-4b14-b668-108240e07b26 · outbound

This paper cites , keywords =.

The complex stellar system M 22: confirming abundance variations with high precision differential measurements , keywords =

Reference 58

Resolution: verified exact; doi, observed 2026-08-02T02:59:24.666085Z

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 d4255298-42a2-4aeb-a50b-b9e8aa188f4e · outbound

This paper cites Royal Observatory Annals , keywords =.

The complex stellar system M 22: confirming abundance variations with high precision differential measurements Royal Observatory Annals , keywords =

Reference 59

Resolution: unresolved; no resolver link, observed 2026-08-02T02:58:15.938587Z

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Unavailable: canonical work link unavailable.

Observation a81f1f98-c5b3-402e-ac5a-383127c72400 · outbound

This paper cites an unresolved cited work.

The complex stellar system M 22: confirming abundance variations with high precision differential measurements Unresolved cited work

Reference 60

Resolution: verified exact; doi, observed 2026-08-02T02:59:24.453149Z

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 69795d98-8f4b-494d-9461-8e936bd53cea · outbound

This paper cites an unresolved cited work.

The complex stellar system M 22: confirming abundance variations with high precision differential measurements Unresolved cited work

Reference 61

Resolution: verified exact; doi, observed 2026-08-02T02:59:24.244270Z

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 5c963cde-4cd0-4d72-94e7-f29eb1e0bf47 · outbound

This paper cites , keywords =.

The complex stellar system M 22: confirming abundance variations with high precision differential measurements , keywords =

Reference 62

Resolution: unresolved; no resolver link, observed 2026-08-02T02:58:15.945102Z

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Unavailable: canonical work link unavailable.

Observation 59830fee-4730-4e11-ba31-19bdba3496f8 · outbound

This paper cites , keywords =.

The complex stellar system M 22: confirming abundance variations with high precision differential measurements , keywords =

Reference 63

Resolution: unresolved; no resolver link, observed 2026-08-02T02:58:15.947347Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 0bb6c804-68f0-4b8e-bb73-08dedb74c400 · outbound

This paper cites , keywords =.

The complex stellar system M 22: confirming abundance variations with high precision differential measurements , keywords =

Reference 64

Resolution: unresolved; no resolver link, observed 2026-08-02T02:58:15.949383Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 0c187b10-0cb6-455f-82f3-bfd99cd8fd86 · outbound

This paper cites , keywords =.

The complex stellar system M 22: confirming abundance variations with high precision differential measurements , keywords =

Reference 65

Resolution: verified exact; doi, observed 2026-08-02T02:59:24.071732Z

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 6319520d-4c08-4175-b007-8218c827345c · outbound

This paper cites Vistas in Astronomy , year = 1956, month = jan, volume =.

The complex stellar system M 22: confirming abundance variations with high precision differential measurements Vistas in Astronomy , year = 1956, month = jan, volume =

Reference 66

Resolution: verified exact; doi, observed 2026-08-02T02:59:23.869509Z

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 02c9db03-29e6-40ae-817e-bcfe0ee98733 · outbound

This paper cites , year = 1961, month = mar, volume =.

The complex stellar system M 22: confirming abundance variations with high precision differential measurements , year = 1961, month = mar, volume =

Reference 67

Resolution: verified exact; doi, observed 2026-08-02T02:59:23.663439Z

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 279f6831-478f-4a0a-9453-7421d7e802d7 · outbound

This paper cites Rotating Globular Clusters.

The complex stellar system M 22: confirming abundance variations with high precision differential measurements Rotating Globular Clusters

Reference 68

Resolution: unresolved; no resolver link, observed 2026-08-02T02:58:15.957450Z

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Unavailable: canonical work link unavailable.

Observation e757e1e4-a3ee-4229-9e58-49a0f1d80cc9 · outbound

This paper cites The internal rotation of globular clusters revealed by Gaia DR2.

The complex stellar system M 22: confirming abundance variations with high precision differential measurements The internal rotation of globular clusters revealed by Gaia DR2

Reference 69

Resolution: unresolved; no resolver link, observed 2026-08-02T02:58:15.959401Z

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Unavailable: canonical work link unavailable.

Observation 52fa7ecf-ad96-424f-9504-02f2d763e448 · outbound

This paper cites A stellar census in globular clusters with MUSE: The contribution of rotation to cluster dynamics studied with 200 000 stars.

The complex stellar system M 22: confirming abundance variations with high precision differential measurements A stellar census in globular clusters with MUSE: The contribution of rotation to cluster dynamics studied with 200 000 stars

Reference 70

Resolution: unresolved; no resolver link, observed 2026-08-02T02:58:15.961406Z

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Unavailable: canonical work link unavailable.

Observation de5201e5-cb34-48f4-9178-08f95a5970ee · outbound

This paper cites Three-Component Kinematics of Multiple Stellar Populations in Globular Clusters with Gaia and VLT.

The complex stellar system M 22: confirming abundance variations with high precision differential measurements Three-Component Kinematics of Multiple Stellar Populations in Globular Clusters with Gaia and VLT

Reference 71

Resolution: unresolved; no resolver link, observed 2026-08-02T02:58:15.963702Z

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Unavailable: canonical work link unavailable.

Observation 99e0cd23-f295-4481-892e-63e5ff93f9d0 · outbound

This paper cites Iron and s-elements abundance variations in NGC5286: comparison with anomalous globular clusters and Milky Way satellites.

The complex stellar system M 22: confirming abundance variations with high precision differential measurements Iron and s-elements abundance variations in NGC5286: comparison with anomalous globular clusters and Milky Way satellites

Reference 72

Resolution: unresolved; no resolver link, observed 2026-08-02T02:58:15.965836Z

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Unavailable: canonical work link unavailable.

Observation 893a6c98-450b-4797-bd0f-abd007f5fce4 · outbound

This paper cites An abundance analysis of bright giants in the globular cluster NGC 1851.

The complex stellar system M 22: confirming abundance variations with high precision differential measurements An abundance analysis of bright giants in the globular cluster NGC 1851

Reference 73

Resolution: unresolved; no resolver link, observed 2026-08-02T02:58:15.967798Z

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Unavailable: canonical work link unavailable.

Observation 55cb0e02-c4e1-47d7-9071-c1352e496689 · outbound

This paper cites Iron and neutron-capture element abundance variations in the globular cluster M2 (NGC 7089).

The complex stellar system M 22: confirming abundance variations with high precision differential measurements Iron and neutron-capture element abundance variations in the globular cluster M2 (NGC 7089)

Reference 74

Resolution: unresolved; no resolver link, observed 2026-08-02T02:58:15.969767Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 8890b2f1-f870-4ee1-a202-90f2c672f1bb · outbound

This paper cites , keywords =.

The complex stellar system M 22: confirming abundance variations with high precision differential measurements , keywords =

Reference 75

Resolution: unresolved; no resolver link, observed 2026-08-02T02:58:15.971844Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation add9cabe-bd9d-4c0e-8db2-b65f54de251c · outbound

This paper cites A catalogue of masses, structural parameters and velocity dispersion profiles of 112 Milky Way globular clusters.

The complex stellar system M 22: confirming abundance variations with high precision differential measurements A catalogue of masses, structural parameters and velocity dispersion profiles of 112 Milky Way globular clusters

Reference 76

Resolution: unresolved; no resolver link, observed 2026-08-02T02:58:15.973636Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ca65f7a1-dc1e-496f-a041-b9b3ef848faf · outbound

This paper cites The Gaia-ESO Survey: Kinematics of seven Galactic globular clusters.

The complex stellar system M 22: confirming abundance variations with high precision differential measurements The Gaia-ESO Survey: Kinematics of seven Galactic globular clusters

Reference 77

Resolution: unresolved; no resolver link, observed 2026-08-02T02:58:15.976079Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f9d24e60-d6ad-4652-8d4b-3a9f426cb558 · outbound

This paper cites an unresolved cited work.

The complex stellar system M 22: confirming abundance variations with high precision differential measurements Unresolved cited work

Reference 78

Resolution: unresolved; no resolver link, observed 2026-08-02T02:58:15.979157Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d3d8750b-a346-46a9-a871-dfab9bd5e230 · outbound

This paper cites an unresolved cited work.

The complex stellar system M 22: confirming abundance variations with high precision differential measurements Unresolved cited work

Reference 79

Resolution: unresolved; no resolver link, observed 2026-08-02T02:58:15.983098Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 9388b28d-59db-47c6-98fd-10fc112f7488 · outbound

This paper cites , year = 1959, month = feb, volume =.

The complex stellar system M 22: confirming abundance variations with high precision differential measurements , year = 1959, month = feb, volume =

Reference 80

Resolution: verified exact; doi, observed 2026-08-02T02:59:23.458920Z

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 4b2b7f93-12a3-4e31-8800-7925a04ffb74 · outbound

This paper cites Harvard College Observatory Bulletin , year = 1930, month = mar, volume =.

The complex stellar system M 22: confirming abundance variations with high precision differential measurements Harvard College Observatory Bulletin , year = 1930, month = mar, volume =

Reference 81

Resolution: unresolved; no resolver link, observed 2026-08-02T02:58:15.989106Z

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Unavailable: canonical work link unavailable.

Observation 66ad8f57-78b7-4e28-adf4-15f859979b30 · outbound

This paper cites Publications of the David Dunlap Observatory , keywords =.

The complex stellar system M 22: confirming abundance variations with high precision differential measurements Publications of the David Dunlap Observatory , keywords =

Reference 82

Resolution: unresolved; no resolver link, observed 2026-08-02T02:58:15.992834Z

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Unavailable: canonical work link unavailable.

Observation 62aad18a-7171-4104-abd1-a4f1e573ad73 · outbound

This paper cites an unresolved cited work.

The complex stellar system M 22: confirming abundance variations with high precision differential measurements Unresolved cited work

Reference 83

Resolution: unresolved; no resolver link, observed 2026-08-02T02:58:15.995001Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 2d34fe3d-1193-49f4-8d03-2652da9f4ad8 · outbound

This paper cites The cluster Terzan 5 as a remnant of a primordial building block of the Galactic bulge.

The complex stellar system M 22: confirming abundance variations with high precision differential measurements The cluster Terzan 5 as a remnant of a primordial building block of the Galactic bulge

Reference 84

Resolution: unresolved; no resolver link, observed 2026-08-02T02:58:15.996804Z

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Unavailable: canonical work link unavailable.

Observation f97761d1-d92c-4a54-9c4e-2f48c77f4417 · outbound

This paper cites Detailed abundances of a large sample of giant stars in M 54 and in the Sagittarius nucleus.

The complex stellar system M 22: confirming abundance variations with high precision differential measurements Detailed abundances of a large sample of giant stars in M 54 and in the Sagittarius nucleus

Reference 85

Resolution: unresolved; no resolver link, observed 2026-08-02T02:58:15.998730Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 9b4833aa-8d14-44b9-94da-1c61bea4d0da · outbound

This paper cites , keywords =.

The complex stellar system M 22: confirming abundance variations with high precision differential measurements , keywords =

Reference 86

Resolution: verified exact; doi, observed 2026-08-02T02:59:23.290841Z

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 6ad8d04e-4d08-48c2-82d2-dd7a51fd2c54 · outbound

This paper cites The Accreted Nuclear Clusters of the Milky Way.

The complex stellar system M 22: confirming abundance variations with high precision differential measurements The Accreted Nuclear Clusters of the Milky Way

Reference 87

Resolution: unresolved; no resolver link, observed 2026-08-02T02:58:16.002476Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f28abc5a-798b-4e87-93d4-0823d05c62d3 · outbound

This paper cites A chemical trompe-l'\oe{}il: no iron spread in the globular cluster M22.

The complex stellar system M 22: confirming abundance variations with high precision differential measurements A chemical trompe-l'\oe{}il: no iron spread in the globular cluster M22

Reference 88

Resolution: unresolved; no resolver link, observed 2026-08-02T02:58:16.004599Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 30c8196b-8f74-49bf-a056-0833258e4880 · outbound

This paper cites Homogeneous Analysis of Globular Clusters from the APOGEE Survey with the BACCHUS Code. II. The Southern Clusters and Overview.

The complex stellar system M 22: confirming abundance variations with high precision differential measurements Homogeneous Analysis of Globular Clusters from the APOGEE Survey with the BACCHUS Code. II. The Southern Clusters and Overview

Reference 89

Resolution: unresolved; no resolver link, observed 2026-08-02T02:58:16.006884Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c6dff1fa-ae44-4428-a27e-4a04f45fa94e · outbound

This paper cites Spectral Evolution of Galaxies , year = 1986, publisher =.

The complex stellar system M 22: confirming abundance variations with high precision differential measurements Spectral Evolution of Galaxies , year = 1986, publisher =

Reference 90

Resolution: unresolved; no resolver link, observed 2026-08-02T02:58:16.009851Z

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Unavailable: canonical work link unavailable.

Observation d9ec9748-2c4a-4eca-b8a9-4d72f4759545 · outbound

This paper cites A new model for the multiple stellar populations within Terzan 5.

The complex stellar system M 22: confirming abundance variations with high precision differential measurements A new model for the multiple stellar populations within Terzan 5

Reference 91

Resolution: unresolved; no resolver link, observed 2026-08-02T02:58:16.012112Z

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Unavailable: canonical work link unavailable.

Observation 4e309697-cd59-4231-99af-4223635c819e · outbound

This paper cites Simulations of globular clusters within their parent galaxies: multiple stellar populations and internal kinematics.

The complex stellar system M 22: confirming abundance variations with high precision differential measurements Simulations of globular clusters within their parent galaxies: multiple stellar populations and internal kinematics

Reference 92

Resolution: unresolved; no resolver link, observed 2026-08-02T02:58:16.014118Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c7430d69-98f2-4fa3-8233-045d39fd7ded · outbound

This paper cites Multiple Stellar Populations in Globular Clusters.

The complex stellar system M 22: confirming abundance variations with high precision differential measurements Multiple Stellar Populations in Globular Clusters

Reference 93

Resolution: unresolved; no resolver link, observed 2026-08-02T02:58:16.016935Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 34d662b8-d43f-4574-a18c-fff48773f505 · outbound

This paper cites , keywords =.

The complex stellar system M 22: confirming abundance variations with high precision differential measurements , keywords =

Reference 94

Resolution: unresolved; no resolver link, observed 2026-08-02T02:58:16.020026Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 90ea660c-9613-401e-85f0-dd27b4aceee8 · outbound

This paper cites , keywords =.

The complex stellar system M 22: confirming abundance variations with high precision differential measurements , keywords =

Reference 95

Resolution: verified exact; doi, observed 2026-08-02T02:59:23.134007Z

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 62e2330d-d9ca-4009-8f6b-c8b546f50fe7 · outbound

This paper cites , keywords =.

The complex stellar system M 22: confirming abundance variations with high precision differential measurements , keywords =

Reference 96

Resolution: unresolved; no resolver link, observed 2026-08-02T02:58:16.024130Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 8979e014-ba8b-42c9-9cde-820d7b85346c · outbound

This paper cites , year = 1980, month = jan, volume =.

The complex stellar system M 22: confirming abundance variations with high precision differential measurements , year = 1980, month = jan, volume =

Reference 97

Resolution: unresolved; no resolver link, observed 2026-08-02T02:58:16.026033Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 3d491cd0-64a9-4ae5-bb03-6753e0e5bb4f · outbound

This paper cites an unresolved cited work.

The complex stellar system M 22: confirming abundance variations with high precision differential measurements Unresolved cited work

Reference 98

Resolution: unresolved; no resolver link, observed 2026-08-02T02:58:16.027762Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 76e2ea70-6519-4bad-aef0-601543118c70 · outbound

This paper cites arXiv e-prints , keywords =.

The complex stellar system M 22: confirming abundance variations with high precision differential measurements arXiv e-prints , keywords =

Reference 99

Resolution: unresolved; no resolver link, observed 2026-08-02T02:58:16.029560Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 631cfacb-d215-4dab-ada5-cdd0970a90ff · outbound

This paper cites The Messenger , year = 2012, month = mar, volume =.

The complex stellar system M 22: confirming abundance variations with high precision differential measurements The Messenger , year = 2012, month = mar, volume =

Reference 100

Resolution: unresolved; no resolver link, observed 2026-08-02T02:58:16.031491Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 1b8db958-eec8-491b-8a92-abc6c74f304b · outbound

This paper cites The Apache Point Observatory Galactic Evolution Experiment (APOGEE).

The complex stellar system M 22: confirming abundance variations with high precision differential measurements The Apache Point Observatory Galactic Evolution Experiment (APOGEE)

Reference 101

Resolution: unresolved; no resolver link, observed 2026-08-02T02:58:16.033529Z

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