J/A+A/535/A2ivo://CDS.VizieR/J/A+A/535/A2doi:10.26093/cds/vizier.35350002CDSBelloche A.Parise B.Schuller F.Andre P.Bontemps S.Menten K.M.CDS support team

CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France

cds-question@unistra.frinterstellar-mediummolecular-cloudsprotostarsyoung-stellar-objectsThe 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.2011A&A...535A...2Bhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/535/A2CatalogResearchIsServedByTAP VizieR generic servicerelated-toJ/A+A/527/A145 : Chamaeleon I 870um sources (Belloche+, 2011)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/535/A2https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/535/A2http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/535/A2https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/535/A2https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/535/A2http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/535/A2GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapOpticaldefault