IRAS08589-4714 molecular gas

DOI

We present an analysis of the region IRAS 08589-4714 with the aim of characterizing the molecular environment. We observed the ^12^CO(3-2), ^13^CO(3-2), C^18^O(3-2), HCO^+^(3-2), and HCN(3-2) molecular lines in a region of 150"x150", centered on the IRAS source, to analyze the distribution and characteristics of the molecular gas linked to the IRAS source.

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Identifier
DOI http://doi.org/10.26093/cds/vizier.35940115
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/A+A/594/A115
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/594/A115
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/594/A115
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/A+A/594/A115
Provenance
Creator Saldano H.P.; Vasquez J.; Cappa C.E.; Gomez M.; Duronea N.; Rubio M.
Publisher CDS
Publication Year 2016
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; Cosmology; Interstellar medium; Natural Sciences; Physics; Stellar Astronomy