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| NGC 6121 369 , the SIMBAD biblio (10 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST06:26:29 |
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More on score
| Bibcode/DOI | Score |
in Title|Abstract| Keywords |
in a table | in teXt, Caption, ... | Nb occurence | Nb objects in ref |
Citations (from ADS) |
Title | First 3 Authors |
|---|---|---|---|---|---|---|---|---|---|
| 1977MNRAS.178..353L | 188 | 4 | Near infrared photometry of globular clusters. VI. The moderately metal poor cluster NGC 6121 (M 4). | LLOYD EVANS T. | |||||
| 1990AJ.....99.1491C | 523 | 98 | Astrometry and photometry in the globular cluster M 4. | CUDWORTH K.M. and REES R. | |||||
| 1993AJ....105..173S | 55 | 31 | CN variations among asymptotic giant branch and horizontal branch stars in the intermediate metallicity globular clusters M5, M4, and NGC 6752. | SMITH G.H. and NORRIS J.E. | |||||
1995ApJ...443..124P 
|
543 | 58 | Radial velocities of stars in the globular cluster M 4 and the cluster distance. | PETERSON R.C., REES R.F. and CUDWORTH K.M. | |||||
|
2018MNRAS.478.1520B
|
16 | D | 1 | 11619 | 300 | A catalogue of masses, structural parameters, and velocity dispersion profiles of 112 Milky Way globular clusters. | BAUMGARDT H. and HILKER M. | ||
| 2019ApJ...870L...7W | 97 | K | D | X | 3 | 8 | ~ | Ultralow-amplitude RR Lyrae stars in M4. | WALLACE J.J., HARTMAN J.D., BAKOS G.A., et al. |
|
2022AJ....163..152S
|
17 | D | 1 | 583193 | 11 | APOGEE Net: An Expanded Spectral Model of Both Low-mass and High-mass Stars. | SPRAGUE D., CULHANE C., KOUNKEL M., et al. | ||
|
2022ApJS..259...35A
|
17 | D | 1 | 611005 | 320 | The Seventeenth Data Release of the Sloan Digital Sky Surveys: Complete Release of MaNGA, MaStar, and APOGEE-2 Data. | ABDURRO'UF, ACCETTA K., AERTS C., et al. | ||
|
2022MNRAS.515.3184H
|
102 | D | F | 3 | 83 | 4 | Integrated mass-loss of evolved stars in M4 using asteroseismology. | HOWELL M., CAMPBELL S.W., STELLO D., et al. | |
|
2025A&A...702A.116M
|
19 | D | 1 | 86 | ~ | Matching seismic masses for RR Lyrae-type and oscillating red horizontal branch stars in M4. | MOLNAR L., NETZEL H., HOWELL M., et al. |
