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Aperture-synthesis observations of H I in the galaxy M82

Journal Article · · Astrophys. J.; (United States)
DOI:https://doi.org/10.1086/156543· OSTI ID:6208131
Maps of neutral hydrogen emission in the irregular galaxy M82 were obtained with a spatial resolution of 1' and a velocity resolution of 10.55 km s/sup -1/. A velocity map with spatial resolution of 1.5' was also constructed. These maps reveal a close association of the H I with optical features, including the filaments extending from the nucleus along the galaxy minor axis. A bar of H I at the east end of the major axis of M82 was found which may be due to interaction with M81. The H I distribution and velocities agree quite well with CO data near the nucleus of M82; however, both the systemic velocity of M82 and the velocity gradient determined from the radio data disagree with optically measured values. As much as 50% of the mass of M82 may be interstellar, and active star formation seems likely. 5 figures.
Research Organization:
Univ. of Illinois, Urbana
OSTI ID:
6208131
Journal Information:
Astrophys. J.; (United States), Journal Name: Astrophys. J.; (United States) Vol. 225:3; ISSN ASJOA
Country of Publication:
United States
Language:
English

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