Extragalactic γ -rays
Abstract
Only a few extragalactic objects have been studied in the γ -ray region of the spectrum. At high energies the COS-B experiment detected emission from the quasar 3C273 while at lower energies the results indicate that the emission from the Seyfert galaxy NGC 4151 is variable. A similar variability may also account for the conflicting reports of line emission from the radio galaxy Cen A. The implication of these and other observations in relation to the possible physical conditions in the nuclei of active galaxies.
- Publication:
-
Philosophical Transactions of the Royal Society of London Series A
- Pub Date:
- June 1981
- DOI:
- 10.1098/rsta.1981.0136
- Bibcode:
- 1981RSPTA.301..577D
- Keywords:
-
- Astronomical Spectroscopy;
- Extragalactic Radio Sources;
- Gamma Ray Astronomy;
- Seyfert Galaxies;
- Active Galactic Nuclei;
- Active Galaxies;
- Black Holes (Astronomy);
- Compton Effect;
- Cos-B Satellite;
- Energy Spectra;
- Quasars;
- Radio Galaxies;
- Astronomy;
- ASTRONOMICAL SPECTROSCOPY;
- EXTRAGALACTIC RADIO SOURCES;
- GAMMA RAY ASTRONOMY;
- SEYFERT GALAXIES;
- ACTIVE GALACTIC NUCLEI;
- ACTIVE GALAXIES;
- BLACK HOLES (ASTRONOMY);
- COMPTON EFFECT;
- COS-B SATELLITE;
- ENERGY SPECTRA;
- QUASARS;
- RADIO GALAXIES