Neutral hydrogen absorption observations of the central region of NGC 3628 |
| |
Authors: | G H J Cole C G Mundell & A Pedlar |
| |
Institution: | University of Manchester, Nuffield Radio Astronomy Laboratories, Jodrell Bank, Macclesfield, Cheshire SK11 9DL,;Department of Astronomy, University of Maryland, College Park, Maryland, MD 20742, USA |
| |
Abstract: | Using MERLIN with 0.2-arcsec resolution we have observed neutral hydrogen absorption against the central region of the starburst galaxy NGC 3628. The central region resolves into ~16 continuum components at 1.4 GHz. From comparison with published 15-GHz data, we infer that these components are supernova remnants, although three components may be consistent with a weak active galactic nucleus. Neutral hydrogen absorption is seen against the continuum emission with column densities ~1022 cm?2. The absorption appears to be from two separate absorbing structures. Assuming a simple morphology, the main velocity structure can be attributed to a ring of neutral gas with a radius 130 pc rotating around a central starburst with a velocity gradient of 1270 km s?1 kpc?1. From simple assumptions, the mass interior to this ring is 0.9 × 109 M⊙. The second absorption structure may represent outflow from the starburst region or a large-scale galactic structure. Alternatively the absorption structure may be non-axisymmetric, such as a bar. |
| |
Keywords: | supernova remnants galaxies: individual: NGC 3628 galaxies: ISM galaxies: starburst radio lines: galaxies |
|
|