The effect of the SED shape on the gamma-ray vs. radio emission dependence in AGNs

Details The effect of the SED shape on the gamma-ray vs. radio emission dependence in AGNs The effect of the SED shape on the gamma-ray vs. radio emission dependence in AGNs

Oct 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001aipc..587..301l&link_type=abstract

GAMMA 2001: Gamma-Ray Astrophysics 2001. AIP Conference Proceedings, Volume 587, pp. 301-303 (2001).

Astronomy and Astrophysics

Astrophysics

1

Radio Sources, Gamma-Ray Sources, Gamma-Ray Bursts, Active And Peculiar Galaxies And Related Systems

Scientific paper

The gamma-ray emission in AGNs is produced at the beginning of radio outbursts and is correlated with the radio emission. The type of the correlation, however, seems to depend on the spectral behavior of the source (low-peaking SED, high-peaking SED). We compared the properties of AGNs with the location of the synchrotron peak and found that there is a sequence in the source properties (e.g., class) that depends on the synchrotron peak frequency. Another connection can be found between the gamma-ray vs. radio emission and source luminosity, and also the Doppler factor. .

Affiliated with

Also associated with

No associations

Rating

The effect of the SED shape on the gamma-ray vs. radio emission dependence in AGNs 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 The effect of the SED shape on the gamma-ray vs. radio emission dependence in AGNs, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The effect of the SED shape on the gamma-ray vs. radio emission dependence in AGNs will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1101731