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Issue A&A
Volume 471, Number 3, September I 2007
Page(s) 805 - 806
Section Extragalactic astronomy
DOI http://dx.doi.org/10.1051/0004-6361:20077369



A&A 471, 805-806 (2007)
DOI: 10.1051/0004-6361:20077369

Comments on a faint old stellar system at 150 kpc

H. Kamaya

Department of Earth and Ocean Sciences, School of Applied Sciences, National Defense Academy of Japan, Yokosuka 239-8686, Japan ( Department of Astronomy, School of Science, Kyoto University, Sakyo-Ku, Kyoto 606-8502, Japan, before 2007 April.)
    e-mail: kamaya@nda.ac.jp

(Received 28 February 2007 / Accepted 2 June 2007 )

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.
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.


Key words: Galaxy: halo -- galaxies: dwarf



© ESO 2007


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