A Parsec-Scale Study of the 5/15 GHz Spectral Indices of the Compact Radio Sources in M82

Details A Parsec-Scale Study of the 5/15 GHz Spectral Indices of the Compact Radio Sources in M82 A Parsec-Scale Study of the 5/15 GHz Spectral Indices of the Compact Radio Sources in M82

2002-07-08

arxiv.org/abs/astro-ph/0207158v1

Mon.Not.Roy.Astron.Soc. 334 (2002) 912

Astronomy and Astrophysics

Astrophysics

Accepted for publication in MNRAS. 15 pages, 9 figures

Scientific paper

10.1046/j.1365-8711.2002.05580.x

Observations of the starburst galaxy, M82, have been made with the VLA in its A-configuration at 15 GHz and MERLIN at 5 GHz enabling a spectral analysis of the compact radio structure on a scale of < 0.1'' (1.6 pc). Crucial to these observations was the inclusion of the Pie Town VLBA antenna, which increased the resolution of the VLA observations by a factor of ~2. A number of the weaker sources are shown to have thermal spectra and are identified as HII regions with emission measures ~10^7 cm^-6 pc. Some of the sources appear to be optically thick at 5 GHz implying even higher emission measures of ~10^8 cm^-6 pc. The number of compact radio sources in M82 whose origin has been determined is now 46, of which 30 are supernova related and the remaining 16 are HII regions. An additional 15 sources are noted, but have yet to be identified, meaning that the total number of compact sources in M82 is at least 61. Also, it is shown that the distribution of HII regions is correlated with the large-scale ionised gas distribution, but is different from the distribution of supernova remnants. In addition, the brightest HII region at (B1950) 09h 51m 42.21s +69 54' 59.2'' shows a spectral index gradient across its resolved structure which we attribute to the source becoming optically thick towards its centre.

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