Red MSX sources in BGPS Virtual Observatory Resource

Authors

1. Schenck D.E.
2. Shirley Y.L.
3. Reiter M.
4. Juneau S.

Published by

CDS

Abstract

We present an analysis of the relation between the star formation rate (SFR) and mass of dense gas in Galactic clumps and nearby galaxies. Using the bolometric luminosity as a measure of SFR and the molecular line luminosity of HCO^+^ (3-2) as a measure of dense gas mass, we find that the relation between SFR and Mdense is approximately linear. This is similar to published results derived using HCN (1-0) as a dense gas tracer.

Keywords

1. radio-sources
2. radio-astronomy

Bibliographic source Bibcode

2011AJ....142...94S

See also HTML

https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/142/94

IVOA Identifier IVOID

ivo://CDS.VizieR/J/AJ/142/94

Document Object Identifer DOI

doi:10.26093/cds/vizier.51420094

Access

Web browser access HTML

https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/AJ/142/94
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/AJ/142/94
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/AJ/142/94

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IVOA Cone Search SCS

For use with a cone search client (e.g., TOPCAT).
https://vizier.cds.unistra.fr/viz-bin/conesearch/J/AJ/142/94/table1?
https://vizier.iucaa.in/viz-bin/conesearch/J/AJ/142/94/table1?
http://vizieridia.saao.ac.za/viz-bin/conesearch/J/AJ/142/94/table1?