CO abundance of 3 globules

DOI

We have studied the ratio of carbon monoxide column density to the extinction A_J_ of background field stars in the direction of three globules: B133, B335, L466. The N(CO) to A_J_ ratios were found to vary from cloud to cloud so that they are larger in B335 than in B133 and L466. These variations are thought to primarily arise from variations of the ratio N(CO)/N(H_2_).

Cone search capability for table J/A+A/421/1087/table1 (Positions observed with SEST and the J band extinctions)

Identifier
DOI http://doi.org/10.26093/cds/vizier.34211087
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/A+A/421/1087
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/421/1087
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/421/1087
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/A+A/421/1087
Provenance
Creator Harjunpaa P.; Lehtinen K.; Haikala L.K.
Publisher CDS
Publication Year 2004
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