Discovery of a Faint Old Stellar System at 150 kpc

Details Discovery of a Faint Old Stellar System at 150 kpc Discovery of a Faint Old Stellar System at 150 kpc

2006-10-29

arxiv.org/abs/astro-ph/0610858v1

Astrophys.J.653:L29-L32,2006

Astronomy and Astrophysics

Astrophysics

7pages, 3 figures, accepted by Astrophysical Journal Letter

Scientific paper

10.1086/510332

We report the detection of a faint old stellar system at $(\alpha,\delta)=(194.29^\circ,~34.32^\circ)$ (SDSS J1257+3419), based on the spatial distribution of bright red-giant branch stars in the Sloan Digital Sky Survey Data Release 4. SDSS J1257+3419 has a half-light radius of $38\pm 12$ pc and an absolute integrated $V$-magnitude of $M_V=-4.8^{+1.4}_{-1.0}$ mag at a heliocentric distance of $150\pm 15$ kpc. A comparison between SDSS J1257+3419 and known Galactic halo objects suggests that SDSS J1257+3419 is either (a) a faint and small dwarf galaxy or (b) a faint and widely extended globular cluster. In the former case, SDSS J1257+3419 could represent an entity of a postulated subhalo of the Milky Way. Further photometric and dynamical study of this stellar system is vital to discriminate these possibilities.

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