Rapporteur paper on high energy gamma-ray astronomy, sessions XG4 and XG5

Details Rapporteur paper on high energy gamma-ray astronomy, sessions XG4 and XG5 Rapporteur paper on high energy gamma-ray astronomy, sessions XG4 and XG5

Aug 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983icrc...12..435p&link_type=abstract

IN: International Cosmic Ray Conference, 18th, Bangalore, India, August 22-September 3, 1983, Invited and Rapporteur Papers. Vol

Astronomy and Astrophysics

Astronomy

Energetic Particles, Gamma Ray Astronomy, Pulsars, X Ray Sources, Cos-B Satellite, Crab Nebula, Energy Bands, Interstellar Magnetic Fields, Interstellar Matter

Scientific paper

Contributions related to the techniques presently used in gamma-ray astronomy are reviewed for the high, very high, and ultrahigh energy regions (3 x 10 to the 6th to 10 the 16 eV). The techniques available, based largely on SAS-2, COS-B, and HEAO-1 data, are classified according to the source. High-energy sources include Cygnus X-3, Crab pulsar and nebula, Vela pulsar, and Geminga and other unidentified COS-B sources. Diffuse high-energy gamma-rays are also considered.

Affiliated with

Also associated with

No associations

Rating

Rapporteur paper on high energy gamma-ray astronomy, sessions XG4 and XG5 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 Rapporteur paper on high energy gamma-ray astronomy, sessions XG4 and XG5, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Rapporteur paper on high energy gamma-ray astronomy, sessions XG4 and XG5 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-748209