A search for IRAS galaxies behind the Taurus molecular clouds.

Details A search for IRAS galaxies behind the Taurus molecular clouds. A search for IRAS galaxies behind the Taurus molecular clouds.

Jul 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995a%26a...299..347c&link_type=abstract

Astronomy and Astrophysics, v.299, p.347

Astronomy and Astrophysics

Astrophysics

5

Surveys, Galaxies: Redshifts, Infrared: Galaxies, Large-Scale Structure Of Universe

Scientific paper

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.

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