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Are gamma-ray novae intrinsically rare or just nearby?

Abstract:
Fermi LAT data revealed classical novae as unexpected gamma-ray sources, yet only 6 of 69 of those optically detected in the first 8 years of Fermi LAT observations were confirmed as > 5? gamma-ray sources. These proceedings outline Monte Carlo simulations in which a population of Galactic novae were simulated based on spatial distributions and R-band magnitudes based on their M31 counterparts. Interstellar extinction was added using a double exponential disc model, and gamma-ray properties were defined based on those of the original 6 gamma-ray novae. We demonstrate that observations are consistent will all classical novae being gamma-ray sources, and that the gamma-ray sky background is the largest inhibitor when discovering these sources. Furthermore, we predict that all classical novae occurring within ? 8 kpc and with m R ? 12 will be detected using the Fermi LAT.
Publication status:
Published
Peer review status:
Peer reviewed

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Institution:
University of Oxford
Department:
Physics; Astrophysics
Role:
Author
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Institution:
University of Oxford
Division:
MPLS
Department:
Physics
Sub department:
Astrophysics
Oxford college:
Exeter College
Role:
Author


Publisher:
Proceedings of Science
Host title:
Proceedings of Science
Journal:
Proceedings of Science More from this journal
Volume:
312
Issue:
7th International Fermi Symposium (IFS2017)
Pages:
1-6
Publication date:
2017-12-12
ISSN:
1824-8039


Pubs id:
pubs:824012
UUID:
uuid:00af3726-0859-41b8-9a31-7ba6c6531983
Local pid:
pubs:824012
Source identifiers:
824012
Deposit date:
2018-02-13

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