Comments on a faint old stellar system at 150 kpc
arXiv:0709.0991 · doi:10.1051/0004-6361:20077369
Abstract
Context.Recent study of SDSS J1257+3419 has revealed that this stellar system is either a faint and small dwarf galaxy or a faint and widely extended globular cluster (see also arXiv:0709.0327 [astro-ph]). Aims.In this short note, the author suggests that this system is one of the smallest dwarf spheroidals (dSphs) in the Milky Way. Methods.We re-examine some observational quantities of this object and check whether it can be bound system. Results. As a result, we find the mass of SDSS J1257+3419 is the lowest of dSphs in the Milky Way, and its mass density is typical of dSphs. Important is that the tidal radius of SDSS J1257+3419 is much larger than its half-light radius. That is, this very small dSph can be bound by its own gravity.
1 figures
References in corpus (5)
- A Faint New Milky Way Satellite in Bootes
- A New Milky Way Dwarf Satellite in Canes Venatici
- Exploring Halo Substructure with Giant Stars: The Dynamics and Metallicity of the Dwarf Spheroidal in Bootes
- On the formation of dwarf galaxies and stellar halos
- Discovery of a Faint Old Stellar System at 150 kpc