Very high energy gamma-ray astronomy

Details Very high energy gamma-ray astronomy Very high energy gamma-ray astronomy

May 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997aipc..412..979c&link_type=abstract

The sixth conference on the intersections of particle and nuclear physcis. AIP Conference Proceedings, Volume 412, pp. 979-986

Astronomy and Astrophysics

Astronomy

Gamma-Ray

Scientific paper

Very high energy (VHE) γ-ray astronomy (E>250 GeV) has, in recent years, established its place as an astrophysical discipline. The growing catalog of galactic and extragalactic sources, and the non-detection of prominent astrophysical objects, have impacted theories ranging from the environments of pulsars and active galactic nuclei (AGN) to the origins of cosmic rays. The current status of the field is reviewed, with particular emphasis on observations of AGN and their implications for AGN emission models.

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