Astronomy and Astrophysics – Astrophysics
Scientific paper
2006-08-21
Astrophys.J.654:897-906,2007
Astronomy and Astrophysics
Astrophysics
10 pages, 8 figures, submitted to the Astrophysical Journal
Scientific paper
10.1086/509718
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.
Barentine John C.
Beers Timothy C.
Bell Eric F.
Belokurov Vasily
Bramich Daniel M.
No associations
LandOfFree
Cats and Dogs, Hair and A Hero: A Quintet of New Milky Way Companions does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Cats and Dogs, Hair and A Hero: A Quintet of New Milky Way Companions, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Cats and Dogs, Hair and A Hero: A Quintet of New Milky Way Companions will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-572634