Compton-synchrotron models for the nucleus of Centaurus A /NGC 5128/

Details Compton-synchrotron models for the nucleus of Centaurus A /NGC 5128/ Compton-synchrotron models for the nucleus of Centaurus A /NGC 5128/

Jul 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975apj...199...49g&link_type=abstract

Astrophysical Journal, vol. 199, July 1, 1975, pt. 1, p. 49-53.

Astronomy and Astrophysics

Astronomy

81

Astronomical Models, Compton Effect, Galactic Nuclei, Synchrotron Radiation, Active Galaxies, Galactic Radiation, Gamma Rays, Microwave Emission, X Ray Astronomy

Scientific paper

Compton-synchrotron models are constructed to account for the observed microwave-through-X-ray spectrum and the recently reported flux of gamma-rays with energies in excess of about 300 GeV from NGC 5128 (Cen A). The spectrum suggests a double source structure in the nucleus of NGC 5128. The gamma-rays arise from inverse Compton scattering of a synchrotron photon spectrum that must extend through X-ray energies. The observed gamma-ray flux and the self-absorbed synchrotron spectra determine the angular sizes, energy densities, and magnetic fields of the source. Such parameters for the sources in the nuclei of active galaxies may enable the eventual description of the source mechanisms to be made. Further implications of the model and possible observations are discussed.

Affiliated with

Also associated with

No associations

Rating

Compton-synchrotron models for the nucleus of Centaurus A /NGC 5128/ 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 Compton-synchrotron models for the nucleus of Centaurus A /NGC 5128/, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Compton-synchrotron models for the nucleus of Centaurus A /NGC 5128/ will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1755054