Interpretation of the galactic radio-continuum and gamma ray emission

Details Interpretation of the galactic radio-continuum and gamma ray emission Interpretation of the galactic radio-continuum and gamma ray emission

Nov 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974csgr.conf..259b&link_type=abstract

In ESRO The Context and Status of Gamma Ray Astronomy p 259-263 (SEE N75-25813 16-93)

Astronomy and Astrophysics

Astronomy

Flux Density, Galactic Radiation, Gamma Rays, Radio Emission, Brightness Temperature, Compton Effect, Cosmic Rays, Emission Spectra, Galactic Structure, Line Spectra, Longitude, Nonthermal Radiation, Radiation Distribution, Spiral Galaxies

Scientific paper

The nonthermal radio-continuum and gamma ray emission of the galactic disc were analyzed using a spiral-arm model of the galaxy. The results for the 408 MHz brightness temperature and the 100 MeV gamma ray line intensity as a function of galactic longitude at b to the 11th power = 0 deg are presented. The observational implications, as well as the uncertainties in the calculations, are briefly discussed. An estimate of the possible range of the inverse Compton contribution to the observed gamma ray flux is made.

Affiliated with

Also associated with

No associations

Rating

Interpretation of the galactic radio-continuum and gamma ray emission 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 Interpretation of the galactic radio-continuum and gamma ray emission, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Interpretation of the galactic radio-continuum and gamma ray emission will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1763597