NGC7538IRS1 and NGC7538S 1.36mm maps

DOI

The nature of embedded accretion disks around forming high-mass stars is one of the missing puzzle pieces for a general understanding of the formation of the most massive and luminous stars. We want to dissect the small-scale structure of the dust continuum and kinematic gas emission toward two of the most prominent high-mass disk candidates.

Cone search capability for table J/A+A/543/A88/fits (List of maps)

Identifier
DOI http://doi.org/10.26093/cds/vizier.35430088
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/A+A/543/A88
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/543/A88
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/543/A88
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/A+A/543/A88
Provenance
Creator Beuther H.; Linz H.; Henning T.
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; Natural Sciences; Observational Astronomy; Physics; Stellar Astronomy