A Synchrotron Radiation Model for Extragalactic Infrared Sources

Details A Synchrotron Radiation Model for Extragalactic Infrared Sources A Synchrotron Radiation Model for Extragalactic Infrared Sources

Nov 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979ap%26ss..66..113f&link_type=abstract

Astrophysics and Space Science, Volume 66, Issue 1, pp.113-120

Astronomy and Astrophysics

Astrophysics

Scientific paper

For a number of extragalactic sources of infrared radiation, for example some quasars and nuclei of Class I Seyfert galaxies that are also radio sources, there is a characteristic maximum in the radiation spectrum atv˜1011 Hz. We discuss a model in which this feature is regarded as intrinsic to the process of electron production, and in which the radiation is produced by the synchrotron mechanism. A two-component version of the model can be employed in the interpretation of the composite radiation spectra of several sources — 3C 84 (NGC 1275), 3C 120 and 3C 273.

Affiliated with

Also associated with

No associations

Rating

A Synchrotron Radiation Model for Extragalactic Infrared 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 A Synchrotron Radiation Model for Extragalactic Infrared Sources, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A Synchrotron Radiation Model for Extragalactic Infrared Sources will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-974218