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CO J = 7 → 6 Emission in the Large Magellanic Cloud

Published online by Cambridge University Press:  30 March 2016

Sungeun Kim ,
Wilfred Walsh ,
Kecheng Xiao ,
Adair P. Lane  and
Antony A. Stark
Sungeun Kim
Affiliation:
Univ. of Massachusetts, Astronomy Department, 710 N. Pleasant St., Amherst, MA 01003
Wilfred Walsh
Affiliation:
Harvard-Smithsonian Center for Astrophysics, 60 Garden St., MS-12, Cambrdige, MA 02138
Kecheng Xiao
Affiliation:
Harvard-Smithsonian Center for Astrophysics, 60 Garden St., MS-12, Cambrdige, MA 02138
Adair P. Lane
Affiliation:
Harvard-Smithsonian Center for Astrophysics, 60 Garden St., MS-12, Cambrdige, MA 02138
Antony A. Stark
Affiliation:
Harvard-Smithsonian Center for Astrophysics, 60 Garden St., MS-12, Cambrdige, MA 02138

Abstract

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We present the first detection of 12CO (J = 7 → 6) emission in the Magellanic Clouds toward the 30 Doradus region using the Antarctic Sub-millimeter Telescope and Remote Observatory (AST/RO).

Type
I. Joint Discussions
Information
Highlights of Astronomy , Volume 13 , 2005 , pp. 860 - 863
Copyright
Copyright © Astronomical Society of Pacific 2005

References

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