Molecular and atomic gas in the LMC. II. Virtual Observatory Resource

Authors

1. Fukui Y.
2. Kawamura A.
3. Wong T.
4. Murai M.
5. Iritani H.
6. Mizuno N.
7. Mizuno Y.,Onishi T.
8. Hughes A.
9. Ott J.
10. Muller E.
11. Staveley-Smith L.
12. Kim S.

Published by

CDS

Abstract

We compare the CO (J=1-0) and HI emission in the Large Magellanic Cloud in three dimensions, i.e., including a velocity axis in addition to the two spatial axes, with the aim of elucidating the physical connection between giant molecular clouds (GMCs) and their surrounding HI gas. The CO(J=1-0) data set is from the second NANTEN CO survey (Fukui et al. 2008, Cat. J/ApJS/178/56) and the HI data set is from the merged Australia Telescope Compact Array (ATCA) and Parkes Telescope surveys (Kim et al. 2003ApJS..148..473K).

Keywords

1. molecular-clouds
2. magellanic-clouds
3. radio-astronomy
4. interstellar-medium

Bibliographic source Bibcode

2009ApJ...705..144F

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IVOA Identifier IVOID

ivo://CDS.VizieR/J/ApJ/705/144

Document Object Identifer DOI

doi:10.26093/cds/vizier.17050144

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