Abstract
We present VLA HI imaging of two actively star forming dwarf galaxies, Haro 2 and Haro 4, and include a map of the CO distribution of Haro 2 obtained with OVRO. We discuss some preliminary results based on the distribution of the neutral and molecular gas and its relation to star formation activity.
Original language | English |
---|---|
Title of host publication | In: Gas and Galaxy Evolution, ASP Conference Proceedings 240 |
Publisher | Astronomical Society of the Pacific |
Pages | 228-9 |
ISBN (Print) | 1-58381-077-3 |
Publication status | Published - 2001 |