We present new VLA C-configuration HI imaging of the Lyman Alpha-emitting starburst galaxies Tol 1924-416 and IRAS 08339+6517. The effective resolution probes neutral gas structures larger than 4.7 kpc in Tol 1924-416, and larger than 8.1 kpc in IRAS 08339+6517. Both systems are revealed to be tidally interacting: Tol 1924-416 with ESO 338-IG04B (6.6 arcminutes = 72 kpc minimum separation), and IRAS 08339+6517 with 2MASX J08380769+6508579 (2.4 arcminutes = 56 kpc minimum separation). The HI emission is extended in these systems, with tidal tails and debris between the target galaxies and their companions. Since Lyman Alpha emission has been detected from both of these primary systems, these observations suggest that the geometry of the ISM is one of the factors affecting the escape fraction of Lyman Alpha emission from starburst environments. Furthermore, these observations argue for the importance of interactions in triggering massive star formation events.
Cite
@article{arxiv.astro-ph/0403191,
title = {Extended Tidal Structure In Two Lyman Alpha-Emitting Starburst Galaxies},
author = {John M. Cannon and Evan D. Skillman and Daniel Kunth and Claus Leitherer and Miguel Mas-Hesse and Goran Ostlin and Artashes Petrosian},
journal= {arXiv preprint arXiv:astro-ph/0403191},
year = {2009}
}