Radio spectra and the Byurakan classification of galaxies

Details Radio spectra and the Byurakan classification of galaxies Radio spectra and the Byurakan classification of galaxies

Apr 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983afz....19..251m&link_type=abstract

(Astrofizika, vol. 19, Apr.-June 1983, p. 251-255) Astrophysics (ISSN 0571-7132), vol. 19, no. 2, Oct. 1983, p. 145-147. Transla

Astronomy and Astrophysics

Astronomy

5

Classifications, Galactic Nuclei, Radio Sources (Astronomy), Radio Spectra, Spiral Galaxies, Flux Density, Histograms

Scientific paper

It is shown that among spiral galaxies whose central parts are classified as 2, 4, 5, and 2s in the Biurakan classification objects with flat radio spectra are encountered much more frequently than among galaxies whose central parts are classified as 1 and 3; conversely, among the latter there is a large excess of objects with steep spectra. The excess of objects with flat spectra among the galaxies of the classes 2, 4, 5, and 2s is one more confirmation of the fact noted earlier that galaxies with central condensations and split, star-like, or semistellar nuclei are in an active phase of development.

Affiliated with

Also associated with

No associations

Rating

Radio spectra and the Byurakan classification of 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 Radio spectra and the Byurakan classification of galaxies, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Radio spectra and the Byurakan classification of galaxies will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1233152