The {lambda}-Orionis ring in CO

DOI

The table shows clump parameters for 130 peaks in CO(J=1->0) emission detected in the Lambda-Orionis ring in the survey of Lang et al. (1998PASA...15...70L). The clumps were isolated using the Clumpfind algorithm of Williams et al. (1994, Cat. ). They are ordered and labelled according to the relative brightness of the peak temperatures within them, so clump 1 contains the emission maximum, but not necessarily the maximum W(CO) or largest mass.

Cone search capability for table J/A+A/357/1001/table2 (Clump parameters)

Identifier
DOI http://doi.org/10.26093/cds/vizier.33571001
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/A+A/357/1001
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/357/1001
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/357/1001
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/A+A/357/1001
Provenance
Creator Lang W.J.; Masheder M.R.W.; Dame T.M.; Thaddeus P.
Publisher CDS
Publication Year 2000
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