WARNING: this service will be deprecated in the coming months.
Please consider using ADS Classic or Bumblebee

VLA HI Imaging of the Extreme Star-Forming Dwarf Galaxy Leo P
Bernstein-Cooper, Elijah ( Macalester College ); Cannon, J. M. ( Macalester College ); Adams, E. A. ( Cornell University ); Giovanelli, R. ( Cornell University ); Haynes, M. P. ( Cornell University ); McQuinn, K. B. ( University of Minnesota ); Rhode, K. L. ( Indiana University ); Salzer, J. J. ( Indiana University ); Skillman, E. D. ( University of Minnesota ) show affiliations
American Astronomical Society, AAS Meeting #221, id.352.07
Published in Jan 2013
The ALFALFA survey recently discovered the galaxy Leo P, one of the most extreme low-mass star-forming dwarf galaxies in the local volume. We present new HI spectral line imaging of Leo P acquired with the Karl G. Jansky Very Large Array (VLA) in the B- and C-configurations. A peak column density of 2.5×1020 cm-2 is detected at 30 arcsecond resolution and is spatially coincident with the optical center. Diffuse, low column density HI emission extends to the Southeast. 40% of the ALFALFA flux was recovered by the C-configuration observations; a substantial fraction of the neutral gas component resides on scales larger than 30 arcseconds. A sparsely sampled rotation curve demonstrates that the neutral gas is kinematically complex on scales of ~100 pc. We estimate the dynamical mass Mdyn = 8×106 DMpc M, where DMpc is the distance in Mpc. This can be compared with the total HI mass, MHI = 3×105 D2Mpc .
(c) 2013: American Astronomical Society