Very high-energy γ-ray observations of novae and dwarf novae with the MAGIC telescopes
Context. In the last five years the Fermi Large Area Telescope (LAT) instrument detected GeV γ-ray emission from five novae. The GeV emission can be interpreted in terms of an inverse Compton process of electrons accelerated in a shock. In this case it is expected that protons in the same conditions...
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Veröffentlicht in: | Astronomy and astrophysics (Berlin) 2015-10, Vol.582, p.A67 |
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Format: | Artikel |
Sprache: | eng |
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