Molecular clumps in W51 giant molecular cloud

DOI

In this paper, we present a catalogue of dense molecular clumps located within the W51 giant molecular cloud (GMC). This work is based on Heterodyne Array Receiver Programme ^13^CO J=3-2 observations of the W51 GMC and uses the automated CLUMPFIND algorithm to decompose the region into a total of 1575 clumps of which 1130 are associated with the W51 GMC. We clearly see the distinct structures of the W51 complex and the high-velocity stream previously reported.

Cone search capability for table J/MNRAS/424/1658/W51clumps (Properties of the clumps identified by CLUMPFIND within the region observed by HARP)

Identifier
DOI http://doi.org/10.26093/cds/vizier.74241658
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/MNRAS/424/1658
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/424/1658
Related Identifier https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/424/1658
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/MNRAS/424/1658
Provenance
Creator Parsons H.; Thompson M.A.; Clark J.S.; Chrysostomou A.
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; Exoplanet Astronomy; Interstellar medium; Natural Sciences; Observational Astronomy; Physics