A very deep IRAS survey. III - VLA observations

Details A very deep IRAS survey. III - VLA observations A very deep IRAS survey. III - VLA observations

Apr 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989apj...339...12h&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 339, April 1, 1989, p. 12-26.

Astronomy and Astrophysics

Astronomy

17

Infrared Sources (Astronomy), Sky Surveys (Astronomy), Starburst Galaxies, Very Large Array (Vla), Infrared Astronomy Satellite, Luminosity, Radiant Flux Density, Radio Emission, Spectral Line Width, Spiral Galaxies

Scientific paper

The 60-micron fluxes and positions of sources (primarily starburst galaxies) found in a deep IRAS survey by Hacking and Houck (1987) are compared with 1.49 HGz maps made by the Very Large Array. The radio results are consistent with radio measurements of brighter IRAS galaxies and provide evidence that infrared cirrus does not contaminate the 60-micron sample. The flux-independent ratio of infrared to radio flux densities implies that the 1.4 GHz luminosity function for spiral galaxies is evolving at less than (1 + z) to the power of 4 relative to the 60-micron luminosity function.

Affiliated with

Also associated with

No associations

Rating

A very deep IRAS survey. III - VLA observations 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 A very deep IRAS survey. III - VLA observations, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A very deep IRAS survey. III - VLA observations will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1735424