Dust properties in LMC molecular clouds Virtual Observatory Resource

Authors

1. Paradis D.
2. Reach W.T.
3. Bernard J.-P.
4. Madden S.
5. Dobashi K.
6. Meixner M.,Onishi T.
7. Kawamura A.
8. Fukui Y.

Published by

CDS

Abstract

The objective of this paper is to construct a catalog providing the dust properties and the star formation efficiency (SFE) of the molecular clouds in the Large Magellanic Cloud (LMC). We use the infrared (IR) data obtained with the Spitzer Space Telescope as part of the "Surveying the Agents of a Galaxy's Evolution" Legacy survey as well as the IRAS data. We also work with extinction (Av) maps of the LMC. A total of 272 molecular clouds have been detected in the LMC in a previous molecular survey, accounting for 230 giant molecular clouds (GMCs) and 42 smaller clouds. We perform correlations between the IR emission/extinction and atomic and molecular gas tracers.

Keywords

1. magellanic-clouds
2. molecular-clouds
3. chemical-abundances

Bibliographic source Bibcode

2011AJ....141...43P

See also HTML

https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/141/43

IVOA Identifier IVOID

ivo://CDS.VizieR/J/AJ/141/43

Document Object Identifer DOI

doi:10.26093/cds/vizier.51410043

Access

IVOA Table Access TAP

https://tapvizier.cds.unistra.fr/TAPVizieR/tap
Run SQL-like queries with TAP-enabled clients (e.g., TOPCAT).

IVOA Cone Search SCS

For use with a cone search client (e.g., TOPCAT).
https://vizier.cds.unistra.fr/viz-bin/conesearch/J/AJ/141/43/clouds?
https://vizier.iucaa.in/viz-bin/conesearch/J/AJ/141/43/clouds?
http://vizieridia.saao.ac.za/viz-bin/conesearch/J/AJ/141/43/clouds?