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Molecular Clouds in the Large and Small Magellanic Clouds

Published online by Cambridge University Press:  14 August 2015

Mónica Rubio
Mónica Rubio*
Affiliation:
Departamento de Astronomía, Universidad de Chile

Abstract

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To determine the distribution of molecular gas in the Large and Small Magellanic Clouds (LMC and SMC), we made complete surveys in the J=1-0 transition of CO, of the central 6°×6° and 3°×2° areas of the LMC and SMC, respectively. The observations were made with the 1.2m Columbia Telescope at Cerro Tololo, which provides and angular resolution of 8.8 arcmin at 115 GHz. The spectral resolution of the surveys was 1.3 km s-1 and the sensitivity in antenna temperature was 0.05 K for the LMC and 0.02 K for the SMC.

Type
Joint Commission Meeting
Information
Highlights of Astronomy , Volume 8: Highlights of Astronomy. As presented at the XXth General Assembly of the IAU, 1988 , 1989 , pp. 599 - 600
Copyright
Copyright © Kluwer 1989

References

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Rubio, M. et al., 1989, In preparation.Google Scholar