JHK photometry near IRAS 06145+1455

DOI

Our goal in this paper is to study stars and molecular gas in the direction of IRAS 06145+1455 (WB89-789). The kinematic distance of the associated molecular cloud is 11.9kpc. With a galactocentric distance of ~20.2kpc, this object is at the edge of the (molecular) disk of the Galaxy. We use near-IR (J, H, K), molecular line-, and dust continuum observations.

Cone search capability for table J/A+A/464/909/table4 (NIR photometry data)

Identifier
DOI http://doi.org/10.26093/cds/vizier.34640909
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/A+A/464/909
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/464/909
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/464/909
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/A+A/464/909
Provenance
Creator Brand J.; Wouterloot J.G.A.
Publisher CDS
Publication Year 2007
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; Observational Astronomy; Physics