IRAS galaxies behind Taurus clouds

DOI

We carried out a complete search for IRAS galaxies in the Taurus molecular cloud region at l=169deg to 177deg and b=-19deg to -12deg. We selected a total number of 36 galaxies and galaxy candidates and looked for the 21-cm H I line in 25 objects; we detected H I emission in five of them including one with previously unknown redshift. The spatial density of IRAS galaxies with cz=4000 to 6000km/s is lower in this region than in the adjacent regions at both sides along galactic longitude, where the Perseus supercluster and the Gemini-Monoceros filament are respectively located.

Cone search capability for table J/A+A/299/347/table2 (IRAS galaxies and galaxy candidates in the Taurus molecular cloud region)

Identifier
DOI http://doi.org/10.26093/cds/vizier.32990347
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/A+A/299/347
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/299/347
Related Identifier https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/299/347
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/A+A/299/347
Provenance
Creator CHAMARAUX P.; KAZES I.; SAITO M.; YAMADA T.; TAKATA T.
Publisher CDS
Publication Year 1997
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; Galactic and extragalactic Astronomy; Natural Sciences; Observational Astronomy; Physics