|
other query modes : |
Identifier query |
Coordinate query |
Criteria query |
Reference query |
Basic query |
Script submission |
TAP |
Output options |
Object types |
Help |
| NGC 5272 157 , the SIMBAD biblio (10 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST00:54:55 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
|
1908AnPar..25....1V |
1572 | ~ | Catalogue de 1571 etoiles contenues dans l'amas globulaire Messier 3 (NGC 5272). | VON ZEIPEL M.H. | |||||
| 1961PZ.....13..239K | 406 | 2 | A study of variable stars in the globular cluster M 3 = NGC 5272. | KUKARKIN B.V. and KUKARKINA N.P. | |||||
| 1989ApJS...71..713S | 392 | 8 | An objective-prism survey for outlying blue horizontal-branch stars in globular clusters. | SANDULEAK N. | |||||
| 1990ApJ...350..603S | 339 | 168 | The vertical height of the horizontal branch: the range in the absolute magnitudes of RR Lyrae stars in a given globular cluster. | SANDAGE A. | |||||
|
1994A&AS..104..161T |
728 | 21 | Proper motion study of the globular cluster M 3. | TUCHOLKE H.-J., SCHOLZ R.-D. and BROSCHE P. | |||||
|
1996ApJS..103..433B |
4186 | 34 | A catalog of candidate field horizontal-branch and A-type stars. II. | BEERS T.C., WILHELM R., DOINIDIS S.P., et al. | |||||
|
2011ApJ...738...79X |
15 | D | 1 | 4986 | 124 | Quantifying kinematic substructure in the Milky Way's stellar halo. | XUE X.-X., RIX H.-W., YANNY B., et al. | ||
|
2019MNRAS.486..378L |
16 | D | 1 | 3682 | 75 | The halo's ancient metal-rich progenitor revealed with BHB stars. | LANCASTER L., KOPOSOV S.E., BELOKUROV V., et al. | ||
| 2019ApJ...882...76B | 16 | D | 1 | 60 | ~ | Galactic gas flows from halo to disk: tomography and kinematics at the Milky Way's disk-halo interface. | BISH H.V., WERK J.K., PROCHASKA J.X., et al. | ||
|
2021A&A...654A.107C |
17 | D | 1 | 57382 | 1 | Clean catalogues of blue horizontal-branch stars using Gaia EDR3. | CULPAN R., PELISOLI I. and GEIER S. |