CO abundance of 3 globules Virtual Observatory Resource

Authors

1. Harjunpaa P.
2. Lehtinen K.
3. Haikala L.K.

Published by

CDS

Abstract

We have studied the ratio of carbon monoxide column density to the extinction A_J_ of background field stars in the direction of three globules: B133, B335, L466. The N(CO) to A_J_ ratios were found to vary from cloud to cloud so that they are larger in B335 than in B133 and L466. These variations are thought to primarily arise from variations of the ratio N(CO)/N(H_2_).

Keywords

1. interstellar-medium
2. molecular-clouds
3. co-line-emission

Bibliographic source Bibcode

2004A&A...421.1087H

See also HTML

https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/421/1087

IVOA Identifier IVOID

ivo://CDS.VizieR/J/A+A/421/1087

Document Object Identifer DOI

doi:10.26093/cds/vizier.34211087

Access

Web browser access HTML

http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/421/1087
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/421/1087
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/421/1087

IVOA Table Access TAP

http://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).
http://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/421/1087/table1?
https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/421/1087/table1?
http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/421/1087/table1?