other query modes : |
Identifier query |
Coordinate query |
Criteria query |
Reference query |
Basic query |
Script submission |
TAP |
Output options |
Object types |
Help |
KMHK 480 , the SIMBAD biblio (9 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.03.28CET15:24:49 |
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 |
---|---|---|---|---|---|---|---|---|---|
1963IrAJ....6...74S | 902 | 93 | A catalogue of clusters in the Large Magellanic Cloud. | SHAPLEY H. and LINDSAY E.M. | |||||
1990A&AS...84..527K | 1766 | 60 | The cluster system of the Large Magellanic Cloud. | KONTIZAS M., MORGAN D.H., HATZIDIMITRIOU D., et al. | |||||
1995A&A...298...39W | 17 | 25 | A study of clusters and field stars in two regions in the Large Magellanic Cloud.II. Colour-magnitude diagrams and luminosity functions. | WESTERLUND B.E., LINDE P. and LYNGA G. | |||||
1995A&AS..110..533L | 7 | 5 | A study of clusters and field stars in two regions in the Large Magellanic Cloud. I. CCD photometry in B and V. | LINDE P., LYNGA G. and WESTERLUND B.E. | |||||
1998A&A...339..385W | 11 | 4 | The distribution of stars in three regions in the northeastern part of the Large Magellanic Cloud. | WESTERLUND B.E., LUNDGREN K., PETTERSSON B., et al. | |||||
1999AJ....117..238B | 6185 | 135 | A revised and extended catalog of Magellanic system clusters, associations, and emission nebulae. II. The Large Magellanic Cloud. | BICA E.L.D., SCHMITT H.R., DUTRA C.M., et al. | |||||
2008MNRAS.389..678B | 15 | D | 1 | 9123 | 164 | A general catalogue of extended objects in the Magellanic System. | BICA E., BONATTO C., DUTRA C.M., et al. | ||
2010A&A...517A..50G | 15 | D | 1 | 1522 | 146 | Ages and luminosities of young SMC/LMC star clusters and the recent star formation history of the clouds. | GLATT K., GREBEL E.K. and KOCH A. | ||
2013ApJ...777...82K | 16 | D | 1 | 106 | 2 | Ks-band luminosity evolution of the asymptotic giant branch population based on star clusters in the Large Magellanic Cloud. | KO Y., LEE M.G. and LIM S. |