1.3mm observations of CrA cluster

DOI

The importance of the physical environment in the evolution of newly formed low-mass stars remains an open question. In particular, radiation from nearby more massive stars may affect both the physical and chemical structure of these kinds of young stars. We constrain the physical characteristics of a group of embedded low-mass protostars in Corona Australis in the vicinity of the young luminous Herbig Be star R CrA.

Cone search capability for table J/A+A/548/A24/fits (List of FITS files)

Identifier
DOI http://doi.org/10.26093/cds/vizier.35480024
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/A+A/548/A24
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/548/A24
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/548/A24
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/A+A/548/A24
Provenance
Creator Lindberg J.E.; Jorgensen J.K.
Publisher CDS
Publication Year 2012
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