On the Continuing Formation of the Andromeda Galaxy: Detection of HI Clouds in the M31 Halo

Details On the Continuing Formation of the Andromeda Galaxy: Detection of HI Clouds in the M31 Halo On the Continuing Formation of the Andromeda Galaxy: Detection of HI Clouds in the M31 Halo

2003-11-25

arxiv.org/abs/astro-ph/0311571v1

Astrophys.J. 601 (2004) L39-L42

Astronomy and Astrophysics

Astrophysics

To appear in ApJ Letters, 11 pages with 3 postscript figures (higher resolution figures are available upon request)

Scientific paper

10.1086/381703

Green Bank Telescope (GBT) 21cm observations have revealed a faint, yet extensive HI cloud population surrounding the Andromeda Galaxy (M31). The newfound objects are likely analogs to the high-velocity HI clouds (HVCs) seen around the Milky Way. At least 20 discrete features are detected within 50 kpc of the M31 disk, with radial velocities that are comparable to those of outer disk rotation. In addition, a filamentary ``halo'' component of at least 30 kpc extent is concentrated at the M31 systemic velocity. Some of the discrete features are organized into elongated systems with velocity continuity, suggestive of tidal streams. The discrete population can be characterized by a steep power-law distribution of number versus HI mass in the range between 10^5 and 10^7 M_sun. The velocity line-width of discrete clouds is correlated with the cloud HI mass: such that if the clouds are gravitationally bound this implies a dark- to HI mass ratio of ~ 100:1. Possible origins for the discrete and ``halo'' M31 features include: a Local Group ``cooling flow'', tidal debris from recent mergers or interactions, and the gaseous counterparts of low mass dark-matter halos.

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