Stellar Velocity Dispersion of the Leo A Dwarf Galaxy
arXiv:0705.1093 · doi:10.1086/519547
Abstract
We measure the first stellar velocity dispersion of the Leo A dwarf galaxy, σ= 9.3 +- 1.3 km/s. We derive the velocity dispersion from the radial velocities of ten young B supergiants and two HII regions in the central region of Leo A. We estimate a projected mass of 8 +- 2.7 x10^7 solar masses within a radius of 2 arcmin, and a mass to light ratio of at least 20 +- 6 M_sun/L_sun. These results imply Leo A is at least ~80% dark matter by mass.
6 pages, accepted to ApJ
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- Hypervelocity Stars III. The Space Density and Ejection History of Main Sequence Stars from the Galactic Center
- Chemistry and Kinematics of the Late-Forming Dwarf Irregular Galaxies Leo A, Aquarius, and Sagittarius DIG
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- Dwarf Irregular Galaxy Leo A. Suprime-Cam Wide-Field Stellar Photometry
- A Panchromatic Study of Massive Stars in the Extremely Metal-Poor Local Group Dwarf Galaxy Leo A
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- The Future of Stellar Populations Studies in the Milky Way and the Local Group