Andromeda XXVIII: A Dwarf Galaxy More Than 350 kpc from Andromeda
arXiv:1110.5903 · doi:10.1088/2041-8205/742/1/L14
Abstract
We report the discovery of a new dwarf galaxy, Andromeda XXVIII, using data from the recently-released SDSS DR8. The galaxy is a likely satellite of Andromeda, and, at a separation of kpc, would be one of the most distant of Andromeda's satellites. Its heliocentric distance is kpc, and analysis of its structure and luminosity show that it has an absolute magnitude of and half-light radius of pc, similar to many other faint Local Group dwarfs. With presently-available imaging we are unable to determine if there is ongoing or recent star formation, which prevents us from classifying it as a dwarf spheroidal or dwarf irregular.
Accepted to ApJ Letters
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