Cats and Dogs, Hair and A Hero: A Quintet of New Milky Way Companions
| dc.creator | Belokurov, V. | |
| dc.creator | Zucker, D. B. | |
| dc.creator | Evans, N. W. | |
| dc.creator | Kleyna, J. T. | |
| dc.creator | Koposov, S. | |
| dc.creator | Hodgkin, S. T. | |
| dc.creator | Irwin, M. J. | |
| dc.creator | Gilmore, G. | |
| dc.creator | Wilkinson, M. I. | |
| dc.creator | Fellhauer, M. | |
| dc.creator | Bramich, D. M. | |
| dc.creator | Hewett, P. C. | |
| dc.creator | Vidrih, S. | |
| dc.creator | De Jong, J. T. A. | |
| dc.creator | Smith, J. A. | |
| dc.creator | Rix, H. -W. | |
| dc.creator | Bell, E. F. | |
| dc.creator | Wyse, R. F. G. | |
| dc.creator | Newberg, H. J. | |
| dc.creator | Mayeur, P. A. | |
| dc.creator | Yanny, B. | |
| dc.creator | Rockosi, C. M. | |
| dc.creator | Gnedin, O. Y. | |
| dc.creator | Schneider, D. P. | |
| dc.creator | Beers, T. C. | |
| dc.creator | Barentine, J. C. | |
| dc.creator | Brewington, H. | |
| dc.creator | Brinkmann, J. | |
| dc.creator | Harvanek, M. | |
| dc.creator | Kleinman, S. J. | |
| dc.creator | Krzesinski, J. | |
| dc.creator | Long, D. | |
| dc.creator | Nitta, A. | |
| dc.creator | Snedden, S. A. | |
| dc.date | 2006-08-21 | |
| dc.date.accessioned | 2026-07-07T11:25:55Z | |
| dc.date.available | 2026-07-07T11:25:55Z | |
| dc.description | We present five new satellites of the Milky Way discovered in Sloan Digital Sky Survey (SDSS) imaging data, four of which were followed-up with either the Subaru or the Isaac Newton Telescopes. They include four probable new dwarf galaxies -- one each in the constellations of Coma Berenices, Canes Venatici, Leo and Hercules -- together with one unusually extended globular cluster, Segue 1. We provide distances, absolute magnitudes, half-light radii and color-magnitude diagrams for all five satellites. The morphological features of the color-magnitude diagrams are generally well described by the ridge line of the old, metal-poor globular cluster M92. In the last two years, a total of ten new Milky Way satellites with effective surface brightness mu_v >~ 28 mag/sq. arcsec have been discovered in SDSS data. They are less luminous, more irregular and appear to be more metal-poor than the previously-known nine Milky Way dwarf spheroidals. The relationship between these objects and other populations is discussed. We note that there is a paucity of objects with half-light radii between ~40 pc and ~ 100 pc. We conjecture that this may represent the division between star clusters and dwarf galaxies. | |
| dc.description | 10 pages, 8 figures, submitted to the Astrophysical Journal | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0608448 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0608448 | |
| dc.identifier | Astrophys.J.654:897-906,2007 | |
| dc.identifier | doi:10.1086/509718 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/195663 | |
| dc.subject | Astrophysics | |
| dc.title | Cats and Dogs, Hair and A Hero: A Quintet of New Milky Way Companions | |
| dc.type | text |