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

Author:

,Abdo A. A.,Ackermann M.,Ajello M.,Atwood W. B.,Baldini L.,Ballet J.,Barbiellini G.,Bastieri D.,Bechtol K.,Bellazzini R.,Berenji B.,Blandford R. D.,Bloom E. D.,Bonamente E.,Borgland A. W.,Bouvier A.,Brandt T. J.,Bregeon J.,Brez A.,Brigida M.,Bruel P.,Buehler R.,Burnett T. H.,Buson S.,Caliandro G. A.,Cameron R. A.,Caraveo P. A.,Carrigan S.,Casandjian J. M.,Cecchi C.,Çelik Ö.,Charles E.,Chaty S.,Chekhtman A.,Cheung C. C.,Chiang J.,Ciprini S.,Claus R.,Cohen-Tanugi J.,Conrad J.,Corbel S.,Corbet R.,DeCesar M. E.,den Hartog P. R.,Dermer C. D.,de Palma F.,Digel S. W.,Donato D.,do Couto e Silva E.,Drell P. S.,Dubois R.,Dubus G.,Dumora D.,Favuzzi C.,Fegan S. J.,Ferrara E. C.,Fortin P.,Frailis M.,Fuhrmann L.,Fukazawa Y.,Funk S.,Fusco P.,Gargano F.,Gasparrini D.,Gehrels N.,Germani S.,Giglietto N.,Giordano F.,Giroletti M.,Glanzman T.,Godfrey G.,Grenier I. A.,Grondin M.-H.,Grove J. E.,Guiriec S.,Hadasch D.,Harding A. K.,Hayashida M.,Hays E.,Healey S. E.,Hill A. B.,Horan D.,Hughes R. E.,Itoh R.,Jean P.,Jóhannesson G.,Johnson A. S.,Johnson R. P.,Johnson T. J.,Johnson W. N.,Kamae T.,Katagiri H.,Kataoka J.,Kerr M.,Knödlseder J.,Koerding E.,Kuss M.,Lande J.,Latronico L.,Lee S.-H.,Lemoine-Goumard M.,Llena Garde M.,Longo F.,Loparco F.,Lott B.,Lovellette M. N.,Lubrano P.,Makeev A.,Mazziotta M. N.,McConville W.,McEnery J. E.,Mehault J.,Michelson P. F.,Mizuno T.,Moiseev A. A.,Monte C.,Monzani M. E.,Morselli A.,Moskalenko I. V.,Murgia S.,Nakamori T.,Naumann-Godo M.,Nestoras I.,Nolan P. L.,Norris J. P.,Nuss E.,Ohno M.,Ohsugi T.,Okumura A.,Omodei N.,Orlando E.,Ormes J. F.,Ozaki M.,Paneque D.,Panetta J. H.,Parent D.,Pelassa V.,Pepe M.,Pesce-Rollins M.,Piron F.,Porter T. A.,Rainò S.,Rando R.,Ray P. S.,Razzano M.,Razzaque S.,Rea N.,Reimer A.,Reimer O.,Reposeur T.,Ripken J.,Ritz S.,Romani R. W.,Roth M.,Sadrozinski H. F.-W.,Sander A.,Saz Parkinson P. M.,Scargle J. D.,Schinzel F. K.,Sgrò C.,Shaw M. S.,Siskind E. J.,Smith D. A.,Smith P. D.,Sokolovsky K. V.,Spandre G.,Spinelli P.,Stawarz Ł.,Strickman M. S.,Suson D. J.,Takahashi H.,Takahashi T.,Tanaka T.,Tanaka Y.,Thayer J. B.,Thayer J. G.,Thompson D. J.,Tibaldo L.,Torres D. F.,Tosti G.,Tramacere A.,Uchiyama Y.,Usher T. L.,Vandenbroucke J.,Vasileiou V.,Vilchez N.,Vitale V.,Waite A. P.,Wallace E.,Wang P.,Winer B. L.,Wolff M. T.,Wood K. S.,Yang Z.,Ylinen T.,Ziegler M.,Maehara H.,Nishiyama K.,Kabashima F.,Bach U.,Bower G. C.,Falcone A.,Forster J. R.,Henden A.,Kawabata K. S.,Koubsky P.,Mukai K.,Nelson T.,Oates S. R.,Sakimoto K.,Sasada M.,Shenavrin V. I.,Shore S. N.,Skinner G. K.,Sokoloski J.,Stroh M.,Tatarnikov A. M.,Uemura M.,Wahlgren G. M.,Yamanaka M.

Abstract

A Nova Source of Gamma Rays Novae are thermonuclear explosions that occur at the surface of a white dwarf when material is pulled onto it from a companion star in a binary system. They are different from supernovae because the explosion does not completely destroy the white dwarf. Novae have not been widely considered as high-energy gamma-ray sources. Using the Fermi Large Area Telescope, Abdo et al. (p. 817 ) now report the detection of a nova explosion in gamma rays. The observations provide evidence for the acceleration to relativistic energies of particles in the shock wave following the explosion.

Publisher

American Association for the Advancement of Science (AAAS)

Subject

Multidisciplinary

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