Astronomy and Astrophysics – Astronomy
Scientific paper
Dec 2005
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aas...20717803m&link_type=abstract
American Astronomical Society Meeting 207, #178.03; Bulletin of the American Astronomical Society, Vol. 37, p.1452
Astronomy and Astrophysics
Astronomy
Scientific paper
We present results of a multiwavelength study of the nearby spiral galaxy M51 (NGC 5194). We have obtained deep, high resolution, multi-frequency radio observations using the Very Large Array. We report the detection of numerous point sources, with 12 radioX-ray counterparts identified from a deep Chandra observation. Most of the radio emission is due to the presence of H ii regions, supernovae, supernova remnants, and X-ray binaries. We report radio and X-ray emission from a region coincident with the position of SN1994I approximately nine years after maximum light.
This research has been supported by the following funding grants: NSF AST-0307279 (JJC), CXC GO1-2092B (CJS,REK,JJC), HST-AR-10669.01 (REK). CJS is a Cottrell Scholar sponsored by Research Corporation.
Cowan John J.
Kilgard Roy E.
Maddox Larry A.
Prestwich Andrea H.
Schinnerer Eva
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