Abstract
We present the first spectroscopic analysis of the faint and compact
stellar system Draco II (Dra II, MV = -2.9 ± 0.8,
r_h=19^{+8}_{-6} pc), recently discovered in the Panoramic Survey
Telescope and Rapid Response System 1 3π survey. The observations,
conducted with DEIMOS on the Keck II telescope, establish some of its
basic characteristics: the velocity data reveal a narrow peak with nine
member stars at a systemic heliocentric velocity <v_rrangle
=-347.6^{+1.7}_{-1.8} km s^{-1}, thereby confirming Dra II is a
satellite of the Milky Way; we infer a velocity dispersion with
σvr = 2.9 ± 2.1 km s-1 (
| Original language | English |
|---|---|
| Journal | Monthly Notices of the Royal Astronomical Society: Letters |
| Volume | 458 |
| Issue number | 1 |
| DOIs | |
| Publication status | Published - 1 May 2016 |
Keywords / Materials (for Non-textual outputs)
- galaxies: individual: Draco II
- galaxies: kinematics and dynamics
- Local Group
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