JCMT Observations of CO(3-2) from M82

Lo, K. Y., Stephens, S., Rosenthal, E., Eales, Stephen Anthony ORCID: https://orcid.org/0000-0002-7394-426X and Wynn-Williams, C. G. 1990. JCMT Observations of CO(3-2) from M82. Presented at: Kona Symposium on Millimetre and Submillimetre Astronomy, Kona, Hawaii, 3-6 October 1988. Published in: Watt, Graeme D. and Webster, Adrian S. eds. Submillimetre Astronomy: Proceedings of the Kona Symposium on Millimetre and Submillimetre Astronomy. Astrophysics and Space Science Library (158) Dordrecht: Springer Netherlands, pp. 211-212. 10.1007/978-94-015-6850-0_77

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Abstract

The inner 500 pc of M82 is a nearby proto-typical starburst region.1 A starburst requires at least three conditions: (i) an adequate supply of gas, (ii) gathering of the gas within the star-burst region, typically ≤ 1 kpc in extent in the nuclear region, and (iii) a triggering mechanism for the onset of star formation throughout the region. It is clearly important to understand the physical conditions of molecular gas in such regions.

Item Type:	Conference or Workshop Item (Paper)
Status:	Published
Schools:	Physics and Astronomy
Subjects:	Q Science > QB Astronomy
Publisher:	Springer Netherlands
ISBN:	9789401568524
Related URLs:	Publisher
Last Modified:	24 Oct 2022 11:48
URI:	https://orca.cardiff.ac.uk/id/eprint/49366

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