Distances of molecular cloud Virtual Observatory Resource

Authors

1. May J.
2. Alvarez H.
3. Bronfman L.

Published by

CDS

Abstract

We have used a deep CO survey (at 115GHz) of the third galactic quadrant (May et al., 1993A&AS...99..105M) to derive the physical properties of molecular clouds in the outer Galaxy. Within the range of this survey, from 194{deg} to 270{deg} in galactic longitude, 177 molecular clouds have been identified beyond 2 kpc from the Sun. Distances have been determined kinematically using the rotation curve of Brand (1986, Ph.D. Thesis, University of Leiden) with R_{sun}_=8.5kpc and {Theta}_{sun}_=220km/s.

Keywords

1. molecular-clouds
2. co-line-emission

Bibliographic source Bibcode

1997A&A...327..325M

See also HTML

https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/327/325

IVOA Identifier IVOID

ivo://CDS.VizieR/J/A+A/327/325

Document Object Identifer DOI

doi:10.26093/cds/vizier.33270325

Access

Web browser access HTML

http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/327/325
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/327/325
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/327/325

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/327/325/table2?
https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/327/325/table2?
http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/327/325/table2?