Dust continuum emission from IRAS sources

DOI

In an ongoing effort to identify and study high-mass protostellar candidates we have observed in various tracers a sample of 235 sources selected from the IRAS Point Source Catalog (Cat. ), mostly with delta<-30{deg}, with the SEST antenna at millimeter wavelengths. The sample contains 142 Low sources and 93 High, which are believed to be in different evolutionary stages. Both sub-samples have been studied in detail by comparing their physical properties and morphologies.

Cone search capability for table J/A+A/447/221/table1 (Observed IRAS sources)

Identifier
DOI http://doi.org/10.26093/cds/vizier.34470221
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/A+A/447/221
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/447/221
Related Identifier https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/447/221
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/A+A/447/221
Provenance
Creator Beltran M.T.; Brand J.; Cesaroni R.; Fontani F.; Pezzuto S.; Testi L.,Molinari S.
Publisher CDS
Publication Year 2007
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; Cosmology; Interstellar medium; Natural Sciences; Physics