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Gamma-ray emission concurrent with the nova in the symbiotic binary V407 Cygni

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, we report the Fermi... Full description

Journal Title: Science (New York N.Y.), 13 August 2010, Vol.329(5993), pp.817-21
Main Author: Abdo, A A
Other Authors: 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 , Celik, O , 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 , Garde, M Llena , 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 , Parkinson, P M Saz , 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
Format: Electronic Article Electronic Article
Language: English
Subjects:
ID: E-ISSN: 1095-9203 ; PMID: 20705855 Version:1 ; DOI: 10.1126/science.1192537
Link: http://pubmed.gov/20705855
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recordid: medline20705855
title: Gamma-ray emission concurrent with the nova in the symbiotic binary V407 Cygni
format: Article
creator:
  • 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
  • Celik, O
  • 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
  • Garde, M Llena
  • 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
  • Parkinson, P M Saz
  • 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
subjects:
  • Astrophysics - High Energy Astrophysical Phenomena
ispartof: Science (New York, N.Y.), 13 August 2010, Vol.329(5993), pp.817-21
description: 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, we report the Fermi Large Area Telescope detection of variable gamma-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 pi(0) decay gamma-rays from proton-proton interactions. Emission involving inverse Compton scattering of the red giant radiation is also considered and is not ruled out.
language: eng
source:
identifier: E-ISSN: 1095-9203 ; PMID: 20705855 Version:1 ; DOI: 10.1126/science.1192537
fulltext: fulltext
issn:
  • 10959203
  • 1095-9203
url: Link


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titleGamma-ray emission concurrent with the nova in the symbiotic binary V407 Cygni
creatorAbdo, 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 ; Celik, O ; 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 ; Garde, M Llena ; 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 ; Parkinson, P M Saz ; 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
ispartofScience (New York, N.Y.), 13 August 2010, Vol.329(5993), pp.817-21
identifier
descriptionNovae 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, we report the Fermi Large Area Telescope detection of variable gamma-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 pi(0) decay gamma-rays from proton-proton interactions. Emission involving inverse Compton scattering of the red giant radiation is also considered and is not ruled out.
languageeng
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0Abdo, A A
1Ackermann, M
2Ajello, M
3Atwood, W B
4Baldini, L
5Ballet, J
6Barbiellini, G
7Bastieri, D
8Bechtol, K
9Bellazzini, R
10Berenji, B
11Blandford, R D
12Bloom, E D
13Bonamente, E
14Borgland, A W
15Bouvier, A
16Brandt, T J
17Bregeon, J
18Brez, A
19Brigida, M
20Bruel, P
21Buehler, R
22Burnett, T H
23Buson, S
24Caliandro, G A
25Cameron, R A
26Caraveo, P A
27Carrigan, S
28Casandjian, J M
29Cecchi, C
30Celik, O
31Charles, E
32Chaty, S
33Chekhtman, A
34Cheung, C C
35Chiang, J
36Ciprini, S
37Claus, R
38Cohen-Tanugi, J
39Conrad, J
40Corbel, S
41Corbet, R
42DeCesar, M E
43den Hartog, P R
44Dermer, C D
45de Palma, F
46Digel, S W
47Donato, D
48do Couto e Silva, E
49Drell, P S
50Dubois, R
51Dubus, G
52Dumora, D
53Favuzzi, C
54Fegan, S J
55Ferrara, E C
56Fortin, P
57Frailis, M
58Fuhrmann, L
59Fukazawa, Y
60Funk, S
61Fusco, P
62Gargano, F
63Gasparrini, D
64Gehrels, N
65Germani, S
66Giglietto, N
67Giordano, F
68Giroletti, M
69Glanzman, T
70Godfrey, G
71Grenier, I A
72Grondin, M-H
73Grove, J E
74Guiriec, S
75Hadasch, D
76Harding, A K
77Hayashida, M
78Hays, E
79Healey, S E
80Hill, A B
81Horan, D
82Hughes, R E
83Itoh, R
84Jean, P
85Jóhannesson, G
86Johnson, A S
87Johnson, R P
88Johnson, T J
89Johnson, W N
90Kamae, T
91Katagiri, H
92Kataoka, J
93Kerr, M
94Knödlseder, J
95Koerding, E
96Kuss, M
97Lande, J
98Latronico, L
99Lee, S-H
100...
titleGamma-ray emission concurrent with the nova in the symbiotic binary V407 Cygni
descriptionNovae 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, we report the Fermi Large Area Telescope detection of variable gamma-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 pi(0) decay gamma-rays from proton-proton interactions. Emission involving inverse Compton scattering of the red giant radiation is also considered and is not ruled out.
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titleGamma-ray emission concurrent with the nova in the symbiotic binary V407 Cygni
authorAbdo, 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 ; Celik, O ; 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 ; Garde, M Llena ; 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 ; Parkinson, P M Saz ; 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
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4Baldini, L
5Ballet, J
6Barbiellini, G
7Bastieri, D
8Bechtol, K
9Bellazzini, R
10Berenji, B
11Blandford, R D
12Bloom, E D
13Bonamente, E
14Borgland, A W
15Bouvier, A
16Brandt, T J
17Bregeon, J
18Brez, A
19Brigida, M
20Bruel, P
21Buehler, R
22Burnett, T H
23Buson, S
24Caliandro, G A
25Cameron, R A
26Caraveo, P A
27Carrigan, S
28Casandjian, J M
29Cecchi, C
30Celik, O
31Charles, E
32Chaty, S
33Chekhtman, A
34Cheung, C C
35Chiang, J
36Ciprini, S
37Claus, R
38Cohen-Tanugi, J
39Conrad, J
40Corbel, S
41Corbet, R
42Decesar, M E
43Den Hartog, P R
44Dermer, C D
45De Palma, F
46Digel, S W
47Donato, D
48Do Couto E Silva, E
49Drell, P S
50Dubois, R
51Dubus, G
52Dumora, D
53Favuzzi, C
54Fegan, S J
55Ferrara, E C
56Fortin, P
57Frailis, M
58Fuhrmann, L
59Fukazawa, Y
60Funk, S
61Fusco, P
62Gargano, F
63Gasparrini, D
64Gehrels, N
65Germani, S
66Giglietto, N
67Giordano, F
68Giroletti, M
69Glanzman, T
70Godfrey, G
71Grenier, I A
72Grondin, M-H
73Grove, J E
74Guiriec, S
75Hadasch, D
76Harding, A K
77Hayashida, M
78Hays, E
79Healey, S E
80Hill, A B
81Horan, D
82Hughes, R E
83Itoh, R
84Jean, P
85Jóhannesson, G
86Johnson, A S
87Johnson, R P
88Johnson, T J
89Johnson, W N
90Kamae, T
91Katagiri, H
92Kataoka, J
93Kerr, M
94Knödlseder, J
95Koerding, E
96Kuss, M
97Lande, J
98Latronico, L
99Lee, S-H
100...
jtitleScience (New York, N.Y.)
toplevelpeer_reviewed
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11Blandford
12Bloom
13Bonamente
14Borgland
15Bouvier
16Brandt
17Bregeon
18Brez
19Brigida
20Bruel
21Buehler
22Burnett
23Buson
24Caliandro
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26Caraveo
27Carrigan
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29Cecchi
30Celik
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32Chaty
33Chekhtman
34Cheung
35Chiang
36Ciprini
37Claus
38Cohen-Tanugi
39Conrad
40Corbel
41Corbet
42Decesar
43Den Hartog
44Dermer
45de Palma
46Digel
47Donato
48Do Couto E Silva
49Drell
50Dubois
51Dubus
52Dumora
53Favuzzi
54Fegan
55Ferrara
56Fortin
57Frailis
58Fuhrmann
59Fukazawa
60Funk
61Fusco
62Gargano
63Gasparrini
64Gehrels
65Germani
66Giglietto
67Giordano
68Giroletti
69Glanzman
70Godfrey
71Grenier
72Grondin
73Grove
74Guiriec
75Hadasch
76Harding
77Hayashida
78Hays
79Healey
80Hill
81Horan
82Hughes
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85Jóhannesson
86Johnson
87Kamae
88Katagiri
89Kataoka
90Kerr
91Knödlseder
92Koerding
93Kuss
94Lande
95Latronico
96Lee
97Lemoine-Goumard
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99Longo
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1Ackermann, M
2Ajello, M
3Atwood, W B
4Baldini, L
5Ballet, J
6Barbiellini, G
7Bastieri, D
8Bechtol, K
9Bellazzini, R
10Berenji, B
11Blandford, R D
12Bloom, E D
13Bonamente, E
14Borgland, A W
15Bouvier, A
16Brandt, T J
17Bregeon, J
18Brez, A
19Brigida, M
20Bruel, P
21Buehler, R
22Burnett, T H
23Buson, S
24Caliandro, G A
25Cameron, R A
26Caraveo, P A
27Carrigan, S
28Casandjian, J M
29Cecchi, C
30Celik, O
31Charles, E
32Chaty, S
33Chekhtman, A
34Cheung, C C
35Chiang, J
36Ciprini, S
37Claus, R
38Cohen-Tanugi, J
39Conrad, J
40Corbel, S
41Corbet, R
42Decesar, M E
43Den Hartog, P R
44Dermer, C D
45de Palma, F
46Digel, S W
47Donato, D
48Do Couto E Silva, E
49Drell, P S
50Dubois, R
51Dubus, G
52Dumora, D
53Favuzzi, C
54Fegan, S J
55Ferrara, E C
56Fortin, P
57Frailis, M
58Fuhrmann, L
59Fukazawa, Y
60Funk, S
61Fusco, P
62Gargano, F
63Gasparrini, D
64Gehrels, N
65Germani, S
66Giglietto, N
67Giordano, F
68Giroletti, M
69Glanzman, T
70Godfrey, G
71Grenier, I A
72Grondin, M-H
73Grove, J E
74Guiriec, S
75Hadasch, D
76Harding, A K
77Hayashida, M
78Hays, E
79Healey, S E
80Hill, A B
81Horan, D
82Hughes, R E
83Itoh, R
84Jean, P
85Jóhannesson, G
86Johnson, A S
87Johnson, R P
88Johnson, T J
89Johnson, W N
90Kamae, T
91Katagiri, H
92Kataoka, J
93Kerr, M
94Knödlseder, J
95Koerding, E
96Kuss, M
97Lande, J
98Latronico, L
99Lee, S-H
100...
atitleGamma-ray emission concurrent with the nova in the symbiotic binary V407 Cygni
jtitleScience (New York, N.Y.)
risdate20100813
volume329
issue5993
spage817
pages817-821
eissn1095-9203
formatjournal
genrearticle
ristypeJOUR
abstractNovae 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, we report the Fermi Large Area Telescope detection of variable gamma-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 pi(0) decay gamma-rays from proton-proton interactions. Emission involving inverse Compton scattering of the red giant radiation is also considered and is not ruled out.
doi10.1126/science.1192537
pmid20705855
issn00368075
oafree_for_read
date2010-08-13