Segue 3: An Old, Extremely Low Luminosity Star Cluster in the Milky Way's Halo
| dc.contributor.author | Fadely, R. | |
| dc.contributor.author | Willman, B. | |
| dc.contributor.author | Geha, M. | |
| dc.contributor.author | Walsh, S | |
| dc.contributor.author | Munoz, R. | |
| dc.contributor.author | Jerjen, H. | |
| dc.contributor.author | Vargas, L. | |
| dc.contributor.author | Da Costa, G. | |
| dc.date.accessioned | 2017-01-30T11:03:02Z | |
| dc.date.available | 2017-01-30T11:03:02Z | |
| dc.date.created | 2014-11-19T01:13:52Z | |
| dc.date.issued | 2011 | |
| dc.identifier.citation | Fadely, R. and Willman, B. and Geha, M. and Walsh, S. and Munoz, R. and Jerjen, H. and Vargas, L. et al. 2011. Segue 3: An Old, Extremely Low Luminosity Star Cluster in the Milky Way's Halo. The Astronomical Journal. 142 (3): pp. 88-1-88-12. | |
| dc.identifier.uri | http://hdl.handle.net/20.500.11937/7869 | |
| dc.publisher | Institute of Physics Publishing, Inc | |
| dc.title | Segue 3: An Old, Extremely Low Luminosity Star Cluster in the Milky Way's Halo | |
| dc.type | Journal Article | |
| dcterms.source.volume | 142 | |
| dcterms.source.number | 3 | |
| dcterms.source.startPage | 88 | |
| dcterms.source.endPage | 1 | |
| dcterms.source.issn | 0004-6256 | |
| dcterms.source.title | The Astronomical Journal | |
| curtin.accessStatus | Fulltext not available |