TRACING COLD HI GAS IN NEARBY, LOW-MASS GALAXIES

We analyze line-of-sight atomic hydrogen (HI) line profiles of 31 nearby, low-mass galaxies selected from the Very Large Array-ACS Nearby Galaxy Survey Treasury (VLA-ANGST) and The HI Nearby Galaxy Survey (THINGS) to trace regions containing cold (T less than or similar to 1400 K) HI from observations with a uniform linear scale of 200 pc beam(-1). Our galaxy sample spans four orders of magnitude in total HI mass and nine magnitudes in M-B. We fit single and multiple component functions to each spectrum to isolate the cold, neutral medium given by a low-dispersion (<6 km s(-1)) component of the spectrum. Most HI spectra are adequately fit by a single Gaussian with a dispersion of 8-12 km s(-1). Cold HI is found in 23 of 27 (similar to 85%) galaxies after a reduction of the sample size due to quality-control cuts. The cold HI contributes similar to 20% of the total line-of-sight flux when found with warm HI. Spectra best fit by a single Gaussian, but dominated by cold HI emission (i.e., have velocity dispersions of <6 km s(-1)), are found primarily beyond the optical radius of the host galaxy. The cold HI is typically found in localized regions and is generally not coincident with the very highest surface density peaks of the global HI distribution (which are usually areas of recent star formation). We find a lower limit for the mass fraction of cold-to-total HI gas of only a few percent in each galaxy.