Infrared properties of dusty elliptical galaxies

Details Infrared properties of dusty elliptical galaxies Infrared properties of dusty elliptical galaxies

Jun 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988acaps...8...48h&link_type=abstract

(Acta Astrophysica Sinica, vol. 8, 1988, p. 48-54) Chinese Astronomy and Astrophysics (ISSN 0275-1062), vol. 12, June 1988, p. 1

Astronomy and Astrophysics

Astronomy

Cosmic Dust, Elliptical Galaxies, Infrared Astronomy, Interstellar Matter, Astronomical Catalogs, Colorimetry, Data Sampling, Visible Spectrum

Scientific paper

From published sources including the IRAS survey, a sample of 6 E and S0 galaxies with dust lanes and a comparative sample of 32 such galaxies without dust lanes were collected. No evidence was found that dusty lanes in ellipticals are sites of intensive star formation with strong IR emission. On the IR two-color diagram, ellipticals without dust lanes are located in the same region as normal galaxies, while some of those with dust lanes are located far from this region; these are often active galaxies.

Affiliated with

Also associated with

No associations

Rating

Infrared properties of dusty elliptical galaxies 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 Infrared properties of dusty elliptical galaxies, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Infrared properties of dusty elliptical galaxies will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1176945