Abstract
We present MERLIN and VLA 21 cm observations of atomic hydrogen (HI) absorption seen against the central region of the starburst galaxy M 82. The dynamics and structure of the HI absorbing gas is compared with molecular (CO) and ionised ([Ne II]) gas in M 82 on arcsecond (15 pc) scales. Although we see clear evidence in our HI observations for the CO `expanding superbubble' discussed by Weiss et al. (1999), we note that this feature can also be interpreted in terms of non-circular motions characteristic of gas dynamics in bars.
Original language | English |
---|---|
Title of host publication | host publication |
Editors | John E Hibbard |
Volume | 240 |
Publication status | Published - 2001 |
Event | Gas and Galaxy Evolution - Duration: 1 Jan 1824 → … http://adsabs.harvard.edu/abs/2001ASPC..240..402P |
Conference
Conference | Gas and Galaxy Evolution |
---|---|
Period | 1/01/24 → … |
Internet address |