Very high and ultra-high-energy gamma-rays from giant molecular clouds

Details Very high and ultra-high-energy gamma-rays from giant molecular clouds Very high and ultra-high-energy gamma-rays from giant molecular clouds

Jun 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991ap%26ss.180..305a&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 180, no. 2, June 1991, p. 305-320.

Astronomy and Astrophysics

Astronomy

26

Cerenkov Counters, Galactic Cosmic Rays, Gamma Ray Astronomy, Molecular Clouds, Relativistic Particles, Bremsstrahlung, Compton Effect, Energetic Particles, Gamma Ray Spectra, Star Formation

Scientific paper

Very high and ultra-high-energy gamma-ray fluxes expected from giant molecular clouds, and the prospects of detection of these fluxes by means of air Cherenkov telescopes and EAS arrays of new generation, are discussed. It is shown that forthcoming VHE and UHE gamma-ray detectors will permit a search for gamma rays from molecular clouds and genetically connect them with star-formation regions.

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