Red MSX sources in BGPS

DOI

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.

Cone search capability for table J/AJ/142/94/table1 (Source properties)

Identifier
DOI http://doi.org/10.26093/cds/vizier.51420094
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/AJ/142/94
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/142/94
Related Identifier https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/AJ/142/94
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/AJ/142/94
Provenance
Creator Schenck D.E.; Shirley Y.L.; Reiter M.; Juneau S.
Publisher CDS
Publication Year 2013
Rights https://cds.unistra.fr/vizier-org/licences_vizier.html
OpenAccess true
Contact CDS support team <cds-question(at)unistra.fr>
Representation
Resource Type Dataset; AstroObjects
Discipline Astrophysics and Astronomy; Cosmology; Natural Sciences; Observational Astronomy; Physics