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Gamma-Ray Emission Concurrent with the Nova in the Symbiotic Binary V407 Cygni

Journal Article · · Science
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Novae are thermonuclear explosions on a white dwarf surface fueled by mass accreted from a companion star. Current physical models posit that shocked expanding gas from the nova shell can produce x-ray emission, but emission at higher energies has not been widely expected. Here in this paper, we report the Fermi Large Area Telescope detection of variable γ-ray emission (0.1 to 10 billion electron volts) from the recently detected optical nova of the symbiotic star V407 Cygni. We propose that the material of the nova shell interacts with the dense ambient medium of the red giant primary and that particles can be accelerated effectively to produce π0 decay γ-rays from proton-proton interactions. Lastly, emission involving inverse Compton scattering of the red giant radiation is also considered and is not ruled out.
Research Organization:
SLAC National Accelerator Lab., Menlo Park, CA (United States)
Sponsoring Organization:
USDOE
Contributing Organization:
The Fermi-LAT Collaboration
Grant/Contract Number:
AC02-76SF00515
OSTI ID:
1357543
Journal Information:
Science, Journal Name: Science Journal Issue: 5993 Vol. 329; ISSN 0036-8075
Publisher:
AAASCopyright Statement
Country of Publication:
United States
Language:
English

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Swift X-Ray Observations of Classical Novae. II. The Super Soft Source sample text January 2011
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