Chamaeleon III 870um sources maps

DOI

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.

Identifier
DOI http://doi.org/10.26093/cds/vizier.35350002
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/A+A/535/A2
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/535/A2
Related Identifier https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/535/A2
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/A+A/535/A2
Provenance
Creator Belloche A.; Parise B.; Schuller F.; Andre P.; Bontemps S.; Menten K.M.
Publisher CDS
Publication Year 2011
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; Interstellar medium; Natural Sciences; Physics; Stellar Astronomy