A Faint New Milky Way Satellite in Bootes
Author(s) -
Vasily Belokurov,
D. B. Zucker,
N. W. Evans,
M. I. Wilkinson,
M. J. Irwin,
S. T. Hodgkin,
D. M. Bramich,
Jonathan Irwin,
G. Gilmore,
Beth Willman,
S. Vidrih,
Heidi Jo Newberg,
Rosemary F. Ġ. Wyse,
M. Fellhauer,
P. C. Hewett,
Nathan Cole,
Eric F. Bell,
Timothy C. Beers,
Constance M. Rockosi,
B. Yanny,
E. K. Grebel,
Donald P. Schneider,
Robert H. Lupton,
John C. Barentine,
H. Brewington,
J. Brinkmann,
M. Harvanek,
S. J. Kleinman,
J. Krzesiński,
Daniel C. Long,
A. Nitta,
J. A. Smith,
S. Snedden
Publication year - 2006
Publication title -
the astrophysical journal
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.376
H-Index - 489
eISSN - 1538-4357
pISSN - 0004-637X
DOI - 10.1086/507324
Subject(s) - milky way , physics , sky , galaxy , satellite galaxy , astrophysics , magnitude (astronomy) , astronomy , dwarf galaxy , satellite , radius , constellation , red giant branch , local group , computer science , metallicity , computer security
In this Letter, we announce the discovery of a new satellite of the Milky Wayin the constellation of Bootes at a distance of 60 kpc. It was found in asystematic search for stellar overdensities in the North Galactic Cap usingSloan Digital Sky Survey Data Release 5 (SDSS DR5). The color-magnitude diagramshows a well-defined turn-off, red giant branch, and extended horizontalbranch. Its absolute magnitude is -5.8, which makes it one of the faintestgalaxies known. The half-light radius is 220 pc. The isodensity contours areelongated and have an irregular shape, suggesting that Boo may be a disrupteddwarf spheroidal galaxy.Comment: ApJ (Letters), in pres
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