Fermi establishes classical novae as a distinct class of gamma-ray sources: The Fermi-LAT collaboration

M. Ermann; M. Ajello; A. Albert; L. Baldini; J. Ballet; G. Barbiellini; D. Bastieri; R. Bellazzini; E. Bissaldi; R. D. Blandford; E. D. Bloom; E. Bottacini; T. J. Brandt; J. Bregeon; P. Bruel; R. Buehler; S. Buson; G. A. Caliandro; R. A. Cameron; M. Caragiulo; P. A. Caraveo; E. Cavazzuti; E. Charles; A. Chekhtman; C. C. Cheung; J. Chiang; G. Chiaro; S. Ciprini; R. Claus; J. Cohen-Tanugi; J. Conrad; S. Corbel; F. D'Ammando; A. De Angelis; P. R. Den Hartog; F. De Palma; C. D. Dermer; R. Desiante; S. W. Digel; L. Di Venere; E. Do Couto E Silva; D. Donato; P. S. Drell; A. Drlica-Wagner; C. Favuzzi; E. C. Ferrara; W. B. Focke; A. Franckowiak; L. Fuhrmann; Y. Fukazawa; P. Fusco; F. Gargano; D. Gasparrini; S. Germani; N. Giglietto; F. Giordano; M. Giroletti; T. Glanzman; G. Godfrey; I. A. Grenier; J. E. Grove; S. Guiriec; D. Hadasch; A. K. Harding; M. Hayashida; E. Hays; J. W. Hewitt; A. B. Hill; X. Hou; P. Jean; T. Jogler; G. Jóhannesson; A. S. Johnson; W. N. Johnson; M. Kerr; J. Knödlseder; M. Kuss; S. Larsson; L. Latronico; M. Lemoine-Goumard; F. Longo; F. Loparco; B. Lott; M. N. Lovellette; P. Lubrano; A. Manfreda; P. Martin; F. Massaro; M. Mayer; M. N. Mazziotta; J. E. McEnery; P. F. Michelson; W. Mitthumsiri; T. Mizuno; M. E. Monzani; A. Morselli; I. V. Moskalenko; S. Murgia; R. Nemmen; E. Nuss; T. Ohsugi; N. Omodei; M. Orienti; E. Orlando; J. F. Ormes; D. Paneque; J. H. Panetta; J. S. Perkins; M. Pesce-Rollins; F. Piron; G. Pivato; T. A. Porter; S. Rainò; R. Rando; M. Razzano; S. Razzaque; A. Reimer; O. Reimer; T. Reposeur; P. M. Saz Parkinson; M. Schaal; A. Schulz; C. Sgrò; E. J. Siskind; G. Spandre; P. Spinelli; Stawarz; D. J. Suson; H. Takahashi; T. Tanaka; J. G. Thayer; J. B. Thayer; D. J. Thompson; L. Tibaldo; M. Tinivella; D. F. Torres; G. Tosti; E. Troja; Y. Uchiyama; G. Vianello; B. L. Winer; M. T. Wolff; D. L. Wood; K. S. Wood; M. Wood; S. Charbonnel; R. H.D. Corbet; I. De Gennaro Aquino; J. P. Edlin; E. Mason; G. J. Schwarz; S. N. Shore; S. Starrfield; F. Teyssier

doi:10.1126/science.1253947

Fermi establishes classical novae as a distinct class of gamma-ray sources: The Fermi-LAT collaboration

M. Ermann
, M. Ajello
, A. Albert
, L. Baldini
, J. Ballet
, G. Barbiellini
, D. Bastieri
, R. Bellazzini
, E. Bissaldi
, R. D. Blandford
, E. D. Bloom
, E. Bottacini
, T. J. Brandt
, J. Bregeon
, P. Bruel
, R. Buehler
, S. Buson
, G. A. Caliandro
, R. A. Cameron
, M. Caragiulo

P. A. Caraveo, E. Cavazzuti, E. Charles, A. Chekhtman, C. C. Cheung, J. Chiang, G. Chiaro, S. Ciprini, R. Claus, J. Cohen-Tanugi, J. Conrad, S. Corbel, F. D'Ammando, A. De Angelis, P. R. Den Hartog, F. De Palma, C. D. Dermer, R. Desiante, S. W. Digel, L. Di Venere, E. Do Couto E Silva, D. Donato, P. S. Drell, A. Drlica-Wagner, C. Favuzzi, E. C. Ferrara, W. B. Focke, A. Franckowiak, L. Fuhrmann, Y. Fukazawa, P. Fusco, F. Gargano, D. Gasparrini, S. Germani, N. Giglietto, F. Giordano, M. Giroletti, T. Glanzman, G. Godfrey, I. A. Grenier, J. E. Grove, S. Guiriec, D. Hadasch, A. K. Harding, M. Hayashida, E. Hays, J. W. Hewitt, A. B. Hill, X. Hou, P. Jean, T. Jogler, G. Jóhannesson, A. S. Johnson, W. N. Johnson, M. Kerr, J. Knödlseder, M. Kuss, S. Larsson, L. Latronico, M. Lemoine-Goumard, F. Longo, F. Loparco, B. Lott, M. N. Lovellette, P. Lubrano, A. Manfreda, P. Martin, F. Massaro, M. Mayer, M. N. Mazziotta, J. E. McEnery, P. F. Michelson, W. Mitthumsiri, T. Mizuno, M. E. Monzani, A. Morselli, I. V. Moskalenko, S. Murgia, R. Nemmen, E. Nuss, T. Ohsugi, N. Omodei, M. Orienti, E. Orlando, J. F. Ormes, D. Paneque, J. H. Panetta, J. S. Perkins, M. Pesce-Rollins, F. Piron, G. Pivato, T. A. Porter, S. Rainò, R. Rando, M. Razzano, S. Razzaque, A. Reimer, O. Reimer, T. Reposeur, P. M. Saz Parkinson, M. Schaal, A. Schulz, C. Sgrò, E. J. Siskind, G. Spandre, P. Spinelli, Stawarz, D. J. Suson, H. Takahashi, T. Tanaka, J. G. Thayer, J. B. Thayer, D. J. Thompson, L. Tibaldo, M. Tinivella, D. F. Torres, G. Tosti, E. Troja, Y. Uchiyama, G. Vianello, B. L. Winer, M. T. Wolff, D. L. Wood, K. S. Wood, M. Wood, S. Charbonnel, R. H.D. Corbet, I. De Gennaro Aquino, J. P. Edlin, E. Mason, G. J. Schwarz, S. N. Shore, S. Starrfield, F. Teyssier

Physics

German Electron Synchrotron
Clemson University
SLAC National Accelerator Laboratory
National Institute for Nuclear Physics
CNRS
University of Trieste
University of Padua
NASA Goddard Space Flight Center
Université Montpellier 2
École polytechnique
Consorzio Interuniversitario per la Fisica Spaziale (CIFS)
Istituto di Astrofisica Spaziale e Fisica Cosmica di Bologna
Italian Space Agency
George Mason University
Naval Research Laboratory
Osservatorio Astronomico Roma
Stockholm University
Oskar Klein Centre
K. A. Wallenberg Foundation
Royal Swedish Academy of Sciences
Institut universitaire de France
National Institute for Astrophysics
University of Bologna
University of Udine
Polytechnic University of Bari
University of Maryland
Fermi National Accelerator Laboratory
Max Planck Institute for Radio Astronomy
Hiroshima University
University of Perugia
NASA Postdoctoral Program Fellow
University of Innsbruck
The University of Tokyo
University of Maryland Baltimore County
University of Southampton
Marie Curie IOF
Centre d'Etudes Nucléaires Bordeaux-Gradingnan (CENBG)
IRAP
Université Toulouse III - Paul Sabatier
University of Iceland
CSIRO
Yale University
Faculty of Science, Mahidol University
University of California at Irvine
University of Denver
Max Planck Institute for Physics (Werner Heisenberg Institute)
University and Research (MIUR)
University of California at Santa Cruz
The University of Hong Kong
National Research Council
NYCB Real-Time Computing Inc.
JAXA Institute of Space and Astronautical Science
Jagiellonian University in Kraków
Purdue University Northwest
Kyoto University
CSIC
ICREA
Ohio State University
Praxis, Inc.
Durtal Observatory
University of Pisa
University of Hamburg
Osservatorio Astronomico di Trieste
American Astronomical Society
Arizona State University

Research output: Contribution to journal › Article › peer-review

197 Citations (Scopus)

Abstract

A classical nova results from runaway thermonuclear explosions on the surface of a white dwarf that accretes matter from a low-mass main-sequence stellar companion. In 2012 and 2013, three novae were detected in γ rays and stood in contrast to the first γ-ray-detected nova V407 Cygni 2010, which belongs to a rare class of symbiotic binary systems. Despite likely differences in the compositions and masses of their white dwarf progenitors, the three classical novae are similarly characterized as soft-spectrum transient γ-ray sources detected over 2- to 3-week durations. The γ-ray detections point to unexpected high-energy particle acceleration processes linked to the mass ejection from thermonuclear explosions in an unanticipated class of Galactic γ-ray sources.

Original language	English
Pages (from-to)	554-558
Number of pages	5
Journal	Science
Volume	345
Issue number	6196
DOIs	https://doi.org/10.1126/science.1253947
Publication status	Published - 1 Aug 2014

ASJC Scopus subject areas

Multidisciplinary

Access to Document

10.1126/science.1253947

Cite this

Ermann, M., Ajello, M., Albert, A., Baldini, L., Ballet, J., Barbiellini, G., Bastieri, D., Bellazzini, R., Bissaldi, E., Blandford, R. D., Bloom, E. D., Bottacini, E., Brandt, T. J., Bregeon, J., Bruel, P., Buehler, R., Buson, S., Caliandro, G. A., Cameron, R. A., ... Teyssier, F. (2014). Fermi establishes classical novae as a distinct class of gamma-ray sources: The Fermi-LAT collaboration. Science, 345(6196), 554-558. https://doi.org/10.1126/science.1253947

@article{1a890eb5036c43ea8303c44ed6119d07,

title = "Fermi establishes classical novae as a distinct class of gamma-ray sources: The Fermi-LAT collaboration",

abstract = "A classical nova results from runaway thermonuclear explosions on the surface of a white dwarf that accretes matter from a low-mass main-sequence stellar companion. In 2012 and 2013, three novae were detected in γ rays and stood in contrast to the first γ-ray-detected nova V407 Cygni 2010, which belongs to a rare class of symbiotic binary systems. Despite likely differences in the compositions and masses of their white dwarf progenitors, the three classical novae are similarly characterized as soft-spectrum transient γ-ray sources detected over 2- to 3-week durations. The γ-ray detections point to unexpected high-energy particle acceleration processes linked to the mass ejection from thermonuclear explosions in an unanticipated class of Galactic γ-ray sources.",

author = "M. Ermann and M. Ajello and A. Albert and L. Baldini and J. Ballet and G. Barbiellini and D. Bastieri and R. Bellazzini and E. Bissaldi and Blandford, \{R. D.\} and Bloom, \{E. D.\} and E. Bottacini and Brandt, \{T. J.\} and J. Bregeon and P. Bruel and R. Buehler and S. Buson and Caliandro, \{G. A.\} and Cameron, \{R. A.\} and M. Caragiulo and Caraveo, \{P. A.\} and E. Cavazzuti and E. Charles and A. Chekhtman and Cheung, \{C. C.\} and J. Chiang and G. Chiaro and S. Ciprini and R. Claus and J. Cohen-Tanugi and J. Conrad and S. Corbel and F. D'Ammando and \{De Angelis\}, A. and \{Den Hartog\}, \{P. R.\} and \{De Palma\}, F. and Dermer, \{C. D.\} and R. Desiante and Digel, \{S. W.\} and \{Di Venere\}, L. and \{Do Couto E Silva\}, E. and D. Donato and Drell, \{P. S.\} and A. Drlica-Wagner and C. Favuzzi and Ferrara, \{E. C.\} and Focke, \{W. B.\} and A. Franckowiak and L. Fuhrmann and Y. Fukazawa and P. Fusco and F. Gargano and D. Gasparrini and S. Germani and N. Giglietto and F. Giordano and M. Giroletti and T. Glanzman and G. Godfrey and Grenier, \{I. A.\} and Grove, \{J. E.\} and S. Guiriec and D. Hadasch and Harding, \{A. K.\} and M. Hayashida and E. Hays and Hewitt, \{J. W.\} and Hill, \{A. B.\} and X. Hou and P. Jean and T. Jogler and G. J{\'o}hannesson and Johnson, \{A. S.\} and Johnson, \{W. N.\} and M. Kerr and J. Kn{\"o}dlseder and M. Kuss and S. Larsson and L. Latronico and M. Lemoine-Goumard and F. Longo and F. Loparco and B. Lott and Lovellette, \{M. N.\} and P. Lubrano and A. Manfreda and P. Martin and F. Massaro and M. Mayer and Mazziotta, \{M. N.\} and McEnery, \{J. E.\} and Michelson, \{P. F.\} and W. Mitthumsiri and T. Mizuno and Monzani, \{M. E.\} and A. Morselli and Moskalenko, \{I. V.\} and S. Murgia and R. Nemmen and E. Nuss and T. Ohsugi and N. Omodei and M. Orienti and E. Orlando and Ormes, \{J. F.\} and D. Paneque and Panetta, \{J. H.\} and Perkins, \{J. S.\} and M. Pesce-Rollins and F. Piron and G. Pivato and Porter, \{T. A.\} and S. Rain{\`o} and R. Rando and M. Razzano and S. Razzaque and A. Reimer and O. Reimer and T. Reposeur and \{Saz Parkinson\}, \{P. M.\} and M. Schaal and A. Schulz and C. Sgr{\`o} and Siskind, \{E. J.\} and G. Spandre and P. Spinelli and Stawarz and Suson, \{D. J.\} and H. Takahashi and T. Tanaka and Thayer, \{J. G.\} and Thayer, \{J. B.\} and Thompson, \{D. J.\} and L. Tibaldo and M. Tinivella and Torres, \{D. F.\} and G. Tosti and E. Troja and Y. Uchiyama and G. Vianello and Winer, \{B. L.\} and Wolff, \{M. T.\} and Wood, \{D. L.\} and Wood, \{K. S.\} and M. Wood and S. Charbonnel and Corbet, \{R. H.D.\} and \{De Gennaro Aquino\}, I. and Edlin, \{J. P.\} and E. Mason and Schwarz, \{G. J.\} and Shore, \{S. N.\} and S. Starrfield and F. Teyssier",

year = "2014",

month = aug,

day = "1",

doi = "10.1126/science.1253947",

language = "English",

volume = "345",

pages = "554--558",

journal = "Science",

issn = "0036-8075",

publisher = "American Association for the Advancement of Science",

number = "6196",

}

Ermann, M, Ajello, M, Albert, A, Baldini, L, Ballet, J, Barbiellini, G, Bastieri, D, Bellazzini, R, Bissaldi, E, Blandford, RD, Bloom, ED, Bottacini, E, Brandt, TJ, Bregeon, J, Bruel, P, Buehler, R, Buson, S, Caliandro, GA, Cameron, RA, Caragiulo, M, Caraveo, PA, Cavazzuti, E, Charles, E, Chekhtman, A, Cheung, CC, Chiang, J, Chiaro, G, Ciprini, S, Claus, R, Cohen-Tanugi, J, Conrad, J, Corbel, S, D'Ammando, F, De Angelis, A, Den Hartog, PR, De Palma, F, Dermer, CD, Desiante, R, Digel, SW, Di Venere, L, Do Couto E Silva, E, Donato, D, Drell, PS, Drlica-Wagner, A, Favuzzi, C, Ferrara, EC, Focke, WB, Franckowiak, A, Fuhrmann, L, Fukazawa, Y, Fusco, P, Gargano, F, Gasparrini, D, Germani, S, Giglietto, N, Giordano, F, Giroletti, M, Glanzman, T, Godfrey, G, Grenier, IA, Grove, JE, Guiriec, S, Hadasch, D, Harding, AK, Hayashida, M, Hays, E, Hewitt, JW, Hill, AB, Hou, X, Jean, P, Jogler, T, Jóhannesson, G, Johnson, AS, Johnson, WN, Kerr, M, Knödlseder, J, Kuss, M, Larsson, S, Latronico, L, Lemoine-Goumard, M, Longo, F, Loparco, F, Lott, B, Lovellette, MN, Lubrano, P, Manfreda, A, Martin, P, Massaro, F, Mayer, M, Mazziotta, MN, McEnery, JE, Michelson, PF, Mitthumsiri, W, Mizuno, T, Monzani, ME, Morselli, A, Moskalenko, IV, Murgia, S, Nemmen, R, Nuss, E, Ohsugi, T, Omodei, N, Orienti, M, Orlando, E, Ormes, JF, Paneque, D, Panetta, JH, Perkins, JS, Pesce-Rollins, M, Piron, F, Pivato, G, Porter, TA, Rainò, S, Rando, R, Razzano, M, Razzaque, S, Reimer, A, Reimer, O, Reposeur, T, Saz Parkinson, PM, Schaal, M, Schulz, A, Sgrò, C, Siskind, EJ, Spandre, G, Spinelli, P, Stawarz, Suson, DJ, Takahashi, H, Tanaka, T, Thayer, JG, Thayer, JB, Thompson, DJ, Tibaldo, L, Tinivella, M, Torres, DF, Tosti, G, Troja, E, Uchiyama, Y, Vianello, G, Winer, BL, Wolff, MT, Wood, DL, Wood, KS, Wood, M, Charbonnel, S, Corbet, RHD, De Gennaro Aquino, I, Edlin, JP, Mason, E, Schwarz, GJ, Shore, SN, Starrfield, S & Teyssier, F 2014, 'Fermi establishes classical novae as a distinct class of gamma-ray sources: The Fermi-LAT collaboration', Science, vol. 345, no. 6196, pp. 554-558. https://doi.org/10.1126/science.1253947

TY - JOUR

T1 - Fermi establishes classical novae as a distinct class of gamma-ray sources

T2 - The Fermi-LAT collaboration

AU - Ermann, M.

AU - Ajello, M.

AU - Albert, A.

AU - Baldini, L.

AU - Ballet, J.

AU - Barbiellini, G.

AU - Bastieri, D.

AU - Bellazzini, R.

AU - Bissaldi, E.

AU - Blandford, R. D.

AU - Bloom, E. D.

AU - Bottacini, E.

AU - Brandt, T. J.

AU - Bregeon, J.

AU - Bruel, P.

AU - Buehler, R.

AU - Buson, S.

AU - Caliandro, G. A.

AU - Cameron, R. A.

AU - Caragiulo, M.

AU - Caraveo, P. A.

AU - Cavazzuti, E.

AU - Charles, E.

AU - Chekhtman, A.

AU - Cheung, C. C.

AU - Chiang, J.

AU - Chiaro, G.

AU - Ciprini, S.

AU - Claus, R.

AU - Cohen-Tanugi, J.

AU - Conrad, J.

AU - Corbel, S.

AU - D'Ammando, F.

AU - De Angelis, A.

AU - Den Hartog, P. R.

AU - De Palma, F.

AU - Dermer, C. D.

AU - Desiante, R.

AU - Digel, S. W.

AU - Di Venere, L.

AU - Do Couto E Silva, E.

AU - Donato, D.

AU - Drell, P. S.

AU - Drlica-Wagner, A.

AU - Favuzzi, C.

AU - Ferrara, E. C.

AU - Focke, W. B.

AU - Franckowiak, A.

AU - Fuhrmann, L.

AU - Fukazawa, Y.

AU - Fusco, P.

AU - Gargano, F.

AU - Gasparrini, D.

AU - Germani, S.

AU - Giglietto, N.

AU - Giordano, F.

AU - Giroletti, M.

AU - Glanzman, T.

AU - Godfrey, G.

AU - Grenier, I. A.

AU - Grove, J. E.

AU - Guiriec, S.

AU - Hadasch, D.

AU - Harding, A. K.

AU - Hayashida, M.

AU - Hays, E.

AU - Hewitt, J. W.

AU - Hill, A. B.

AU - Hou, X.

AU - Jean, P.

AU - Jogler, T.

AU - Jóhannesson, G.

AU - Johnson, A. S.

AU - Johnson, W. N.

AU - Kerr, M.

AU - Knödlseder, J.

AU - Kuss, M.

AU - Larsson, S.

AU - Latronico, L.

AU - Lemoine-Goumard, M.

AU - Longo, F.

AU - Loparco, F.

AU - Lott, B.

AU - Lovellette, M. N.

AU - Lubrano, P.

AU - Manfreda, A.

AU - Martin, P.

AU - Massaro, F.

AU - Mayer, M.

AU - Mazziotta, M. N.

AU - McEnery, J. E.

AU - Michelson, P. F.

AU - Mitthumsiri, W.

AU - Mizuno, T.

AU - Monzani, M. E.

AU - Morselli, A.

AU - Moskalenko, I. V.

AU - Murgia, S.

AU - Nemmen, R.

AU - Nuss, E.

AU - Ohsugi, T.

AU - Omodei, N.

AU - Orienti, M.

AU - Orlando, E.

AU - Ormes, J. F.

AU - Paneque, D.

AU - Panetta, J. H.

AU - Perkins, J. S.

AU - Pesce-Rollins, M.

AU - Piron, F.

AU - Pivato, G.

AU - Porter, T. A.

AU - Rainò, S.

AU - Rando, R.

AU - Razzano, M.

AU - Razzaque, S.

AU - Reimer, A.

AU - Reimer, O.

AU - Reposeur, T.

AU - Saz Parkinson, P. M.

AU - Schaal, M.

AU - Schulz, A.

AU - Sgrò, C.

AU - Siskind, E. J.

AU - Spandre, G.

AU - Spinelli, P.

AU - Stawarz,

AU - Suson, D. J.

AU - Takahashi, H.

AU - Tanaka, T.

AU - Thayer, J. G.

AU - Thayer, J. B.

AU - Thompson, D. J.

AU - Tibaldo, L.

AU - Tinivella, M.

AU - Torres, D. F.

AU - Tosti, G.

AU - Troja, E.

AU - Uchiyama, Y.

AU - Vianello, G.

AU - Winer, B. L.

AU - Wolff, M. T.

AU - Wood, D. L.

AU - Wood, K. S.

AU - Wood, M.

AU - Charbonnel, S.

AU - Corbet, R. H.D.

AU - De Gennaro Aquino, I.

AU - Edlin, J. P.

AU - Mason, E.

AU - Schwarz, G. J.

AU - Shore, S. N.

AU - Starrfield, S.

AU - Teyssier, F.

PY - 2014/8/1

Y1 - 2014/8/1

N2 - A classical nova results from runaway thermonuclear explosions on the surface of a white dwarf that accretes matter from a low-mass main-sequence stellar companion. In 2012 and 2013, three novae were detected in γ rays and stood in contrast to the first γ-ray-detected nova V407 Cygni 2010, which belongs to a rare class of symbiotic binary systems. Despite likely differences in the compositions and masses of their white dwarf progenitors, the three classical novae are similarly characterized as soft-spectrum transient γ-ray sources detected over 2- to 3-week durations. The γ-ray detections point to unexpected high-energy particle acceleration processes linked to the mass ejection from thermonuclear explosions in an unanticipated class of Galactic γ-ray sources.

AB - A classical nova results from runaway thermonuclear explosions on the surface of a white dwarf that accretes matter from a low-mass main-sequence stellar companion. In 2012 and 2013, three novae were detected in γ rays and stood in contrast to the first γ-ray-detected nova V407 Cygni 2010, which belongs to a rare class of symbiotic binary systems. Despite likely differences in the compositions and masses of their white dwarf progenitors, the three classical novae are similarly characterized as soft-spectrum transient γ-ray sources detected over 2- to 3-week durations. The γ-ray detections point to unexpected high-energy particle acceleration processes linked to the mass ejection from thermonuclear explosions in an unanticipated class of Galactic γ-ray sources.

UR - https://www.scopus.com/pages/publications/84905901421

U2 - 10.1126/science.1253947

DO - 10.1126/science.1253947

M3 - Article

AN - SCOPUS:84905901421

SN - 0036-8075

VL - 345

SP - 554

EP - 558

JO - Science

JF - Science

IS - 6196

ER -

Fermi establishes classical novae as a distinct class of gamma-ray sources: The Fermi-LAT collaboration

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