Component separation in the radiation of variable extragalactic sources

Details Component separation in the radiation of variable extragalactic sources Component separation in the radiation of variable extragalactic sources

May 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985afz....22..449h&link_type=abstract

(Astrofizika, vol. 22, May-June 1985, p. 449-460) Astrophysics (ISSN 0571-7132), vol. 22, no. 3, Nov. 1985, p. 264-272. Translat

Statistics

Computation

6

Computational Astrophysics, Extragalactic Radio Sources, Point Sources, Radiant Flux Density, Radiation Distribution, Periodic Variations, Radio Galaxies, Spectral Energy Distribution

Scientific paper

A method of separating the components in the radiation from variable extragalactic sources within the framework of a two-component model is proposed. The components are a normal galaxy and a variable point source with constant energy distribution in the spectrum. After applying the method to a sample of four galaxies, it is concluded that the method is applicable to objects without emission or with faint emission.

Affiliated with

Also associated with

No associations

Rating

Component separation in the radiation of variable extragalactic sources 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 Component separation in the radiation of variable extragalactic sources, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Component separation in the radiation of variable extragalactic sources will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1630531