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Andromeda X, a New Dwarf Spheroidal Satellite of M31: Photometry
Author(s) -
D. B. Zucker,
A. Y. Kniazev,
David MartínezDelgado,
Eric F. Bell,
HansWalter Rix,
E. K. Grebel,
Jon A. Holtzman,
R. A. M. Walterbos,
Constance M. Rockosi,
Donald G. York,
John C. Barentine,
H. Brewington,
J. Brinkmann,
Michael Harvanek,
S. J. Kleinman,
J. Krzesiński,
Dan Long,
Eric H. Neilsen,
A. Nitta,
Stephanie A. Snedden
Publication year - 2007
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 - 10.1086/516748
Subject(s) - andromeda , photometry (optics) , physics , astrophysics , absolute magnitude , local group , astronomy , brightness , andromeda galaxy , sky , apparent magnitude , dwarf spheroidal galaxy , surface brightness , milky way , stars , dwarf galaxy , galaxy , interacting galaxy
We report the discovery of Andromeda X, a new dwarf spheroidal satellite ofM31, based on stellar photometry from the Sloan Digital Sky Survey (SDSS).Using follow-up imaging data we have estimated its distance and other physicalproperties. We find that Andromeda X has a dereddened central surfacebrightness of mu_V,0 ~ 26.7 mag arcsec^-2 and a total apparent magnitude ofV_tot ~ 16.1, which at the derived distance modulus, (m - M)_0 ~ 24.12 - 24.34,yields an absolute magnitude of M_V ~ -8.1 +/- 0.5; these values are quitecomparable to those of Andromeda IX, a previously-discovered low luminosity M31satellite. The discoveries of Andromeda IX and Andromeda X suggest that suchextremely faint satellites may be plentiful in the Local Group.Comment: 4 pages, 4 figures; submitted to Astrophysical Journal Letter

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