SED information for CrA members

DOI

The CrA region and the Coronet cluster form a nearby (138pc), young (1-2Myr) star-forming region that hosts a moderate population of Class I, II, and III objects. We study the structure of the cluster and the properties of the protostars and protoplanetary disks in the region. We present Herschel PACS photometry at 100 and 160um, obtained as part of the Herschel Gould Belt Survey. The Herschel maps reveal the cluster members within the cloud with high sensitivity and high dynamic range.

Cone search capability for table J/A+A/551/A34/stars (List of studied sources (table3, part 1))

Identifier
DOI http://doi.org/10.26093/cds/vizier.35510034
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/A+A/551/A34
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/551/A34
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/551/A34
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/A+A/551/A34
Provenance
Creator Sicilia-Aguilar A.; Henning T.; Linz H.; Andre P.; Stutz A.; Eiroa C.,White G.J.
Publisher CDS
Publication Year 2013
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; Observational Astronomy; Physics; Stellar Astronomy