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| NGC 6656 1057 , the SIMBAD biblio (12 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST22:31:54 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
| 1977A&AS...29..383A | 291 | 35 | The metal-poor globular cluster NGC 6656. | ALCAINO G. | |||||
| 1977ApJ...213..767E | 71 | 43 | The classification of intrinsic variables. VII. The medium-amplitude red variables. | EGGEN O.J. | |||||
| 1978MNRAS.182..293L | 22 | 26 | Membership and other problems of the globular cluster M 22. | LLOYD EVANS T. | |||||
| 1983AJ.....88.1330A | 118 | 28 | The main sequence of the globular cluster M 22. | ALCAINO G. and LILLER W. | |||||
| 1986AJ.....92..348C | 407 | 71 | Proper motions, membership and photometry in the globular cluster M 22. | CUDWORTH K.M. | |||||
|
1994ApJ...420..612P |
132 | 53 | Proper motions and radial velocities in the globular cluster M 22 and the cluster distance. | PETERSON R.C. and CUDWORTH K.M. | |||||
|
1995ApJS...99..637N |
58 | 9 | Equivalent widths for 54 red giants in 47 Tucanae. Ome Centauri, NGC 6397, M22, and NGC 6752. | NORRIS J.E., DA COSTA G.S. and TINGAY S.J. | |||||
| 1996AJ....112..574C | 142 | 39 | Spectroscopic binaries in globular clusters. II. A search for long-period binaries in M22. | COTE P., PRYOR C., McCLURE R.D., et al. | |||||
| 1999A&A...350..476R | 76 | 44 | Stroemgren photometry in globular clusters: M 55 & M 22. | RICHTER P., HILKER M. and RICHTLER T. | |||||
| 2011A&A...532A...8M | 93 | D | C | 5 | 44 | 180 | The two metallicity groups of the globular cluster M 22: a chemical perspective. | MARINO A.F., SNEDEN C., KRAFT R.P., et al. | |
|
2016A&A...591A.118S |
16 | D | 1 | 31408 | 141 | The PASTEL catalogue: 2016 version. | SOUBIRAN C., LE CAMPION J.-F., BROUILLET N., et al. | ||
|
2022A&A...663A...4S |
17 | D | 1 | 14206 | 7 | Assessment of [Fe/H] determinations for FGK stars in spectroscopic surveys. | SOUBIRAN C., BROUILLET N. and CASAMIQUELA L. |