IRAS galaxies behind Taurus clouds (Chamaraux+, 1995)

Details IRAS galaxies behind Taurus clouds (Chamaraux+, 1995) IRAS galaxies behind Taurus clouds (Chamaraux+, 1995)

Nov 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994ycat..32990347c&link_type=abstract

VizieR On-line Data Catalog: J/A+A/299/347. Originally published in: 1995A&A...299..347C

Computer Science

Galaxies: Ir, Radio Sources, Redshifts

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. (1 data file).

Affiliated with

Also associated with

No associations

Rating

IRAS galaxies behind Taurus clouds (Chamaraux+, 1995) does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with IRAS galaxies behind Taurus clouds (Chamaraux+, 1995), we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and IRAS galaxies behind Taurus clouds (Chamaraux+, 1995) will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-950849