Chamaeleon III 870um sources maps Virtual Observatory Resource

Authors

1. Belloche A.
2. Parise B.
3. Schuller F.
4. Andre P.
5. Bontemps S.
6. Menten K.M.

Published by

CDS

Abstract

The nearby Chamaeleon molecular cloud complex is a good laboratory for studying the process of low-mass star formation because it consists of three clouds with very different properties. Chamaeleon III does not show any sign of star formation, while star formation has been very active in Chamaeleon I and may already be finishing. Our goal is to determine whether star formation can proceed in Cha III by searching for prestellar cores, and to compare the results to our recent survey of Cha I.

Keywords

1. interstellar-medium
2. molecular-clouds
3. protostars
4. young-stellar-objects

Bibliographic source Bibcode

2011A&A...535A...2B

See also HTML

https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/535/A2

IVOA Identifier IVOID

ivo://CDS.VizieR/J/A+A/535/A2

Document Object Identifer DOI

doi:10.26093/cds/vizier.35350002

Access

Web browser access HTML

https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/535/A2
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/535/A2
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/535/A2

IVOA Table Access TAP

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