NGC 6334-NGC 6357 complex

DOI

Our knowledge of high-mass star formation has been mainly based on follow-up studies of bright sources found by IRAS, and has thus been incomplete for its earliest phases, which are inconspicuous at infrared wavelengths. With a new generation of powerful bolometer arrays, unbiased large-scale surveys of nearby high-mass star-forming complexes now search for the high-mass analog of low-mass cores and class 0 protostars. Following the pioneering study of Cygnus X, we investigate the star-forming region NGC 6334-NGC 6357 (~1.7kpc)

Cone search capability for table J/A+A/515/A55/table1 (Properties of dense cores detected in NGC 6334-NGC 6357)

Associated data

Identifier
DOI http://doi.org/10.26093/cds/vizier.35150055
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/A+A/515/A55
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/515/A55
Related Identifier https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/515/A55
Related Identifier https://cdsarc.cds.unistra.fr/assocdata/?obs_collection=J/A+A/515/A55
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/A+A/515/A55
Provenance
Creator Russeil D.; Zavagno A.; Motte F.; Schneider N.; Bontemps S.; Walsh A.J.
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; Interdisciplinary Astronomy; Interstellar medium; Natural Sciences; Observational Astronomy; Physics