Periodic emission from the gamma-ray binary 1FGL J1018.6-5856

M. Ackermann; M. Ajello; J. Ballet; G. Barbiellini; D. Bastieri; A. Belfiore; R. Bellazzini; B. Berenji; R. D. Blandford; E. D. Bloom; E. Bonamente; A. W. Borgland; J. Bregeon; M. Brigida; P. Bruel; R. Buehler; S. Buson; G. A. Caliandro; R. A. Cameron; P. A. Caraveo; E. Cavazzuti; C. Cecchi; Ö Çelik; E. Charles; S. Chaty; A. Chekhtman; C. C. Cheung; J. Chiang; S. Ciprini; R. Claus; J. Cohen-Tanugi; S. Corbel; R. H.D. Corbet; S. Cutini; A. De Luca; P. R. Den Hartog; F. De Palma; C. D. Dermer; S. W. Digel; E. Do Couto E Silva; D. Donato; P. S. Drell; A. Drlica-Wagner; R. Dubois; G. Dubus; C. Favuzzi; S. J. Fegan; E. C. Ferrara; W. B. Focke; P. Fortin; Y. Fukazawa; S. Funk; P. Fusco; F. Gargano; D. Gasparrini; N. Gehrels; S. Germani; N. Giglietto; F. Giordano; M. Giroletti; T. Glanzman; G. Godfrey; I. A. Grenier; J. E. Grove; S. Guiriec; D. Hadasch; Y. Hanabata; A. K. Harding; M. Hayashida; E. Hays; A. B. Hill; R. E. Hughes; G. Jóhannesson; A. S. Johnson; T. J. Johnson; T. Kamae; H. Katagiri; J. Kataoka; M. Kerr; J. Knödlseder; M. Kuss; J. Lande; F. Longo; F. Loparco; M. N. Lovellette; P. Lubrano; M. N. Mazziotta; J. E. McEnery; P. F. Michelson; W. Mitthumsiri; T. Mizuno; C. Monte; M. E. Monzani; A. Morselli; I. V. Moskalenko; S. Murgia; T. Nakamori; M. Naumann-Godo; J. P. Norris; E. Nuss; M. Ohno; T. Ohsugi; A. Okumura; N. Omodei; E. Orlando; M. Ozaki; D. Paneque; D. Parent; M. Pesce-Rollins; M. Pierbattista; F. Piron; G. Pivato; T. A. Porter; S. Rainò; R. Rando; M. Razzano; A. Reimer; O. Reimer; S. Ritz; R. W. Romani; M. Roth; P. M. Saz Parkinson; C. Sgrò; E. J. Siskind; G. Spandre; P. Spinelli; 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; T. L. Usher; J. Vandenbroucke; G. Vianello; V. Vitale; A. P. Waite; B. L. Winer; K. S. Wood; M. Wood; Z. Yang; S. Zimmer; M. J. Coe; F. Di Mille; P. G. Edwards; M. D. Filipović; J. L. Payne; J. Stevens; M. A.P. Torres

doi:10.1126/science.1213974

Periodic emission from the gamma-ray binary 1FGL J1018.6-5856

M. Ackermann
, M. Ajello
, J. Ballet
, G. Barbiellini
, D. Bastieri
, A. Belfiore
, R. Bellazzini
, B. Berenji
, R. D. Blandford
, E. D. Bloom
, E. Bonamente
, A. W. Borgland
, J. Bregeon
, M. Brigida
, P. Bruel
, R. Buehler
, S. Buson
, G. A. Caliandro
, R. A. Cameron
, P. A. Caraveo

E. Cavazzuti, C. Cecchi, Ö Çelik, E. Charles, S. Chaty, A. Chekhtman, C. C. Cheung, J. Chiang, S. Ciprini, R. Claus, J. Cohen-Tanugi, S. Corbel, R. H.D. Corbet, S. Cutini, A. De Luca, P. R. Den Hartog, F. De Palma, C. D. Dermer, S. W. Digel, E. Do Couto E Silva, D. Donato, P. S. Drell, A. Drlica-Wagner, R. Dubois, G. Dubus, C. Favuzzi, S. J. Fegan, E. C. Ferrara, W. B. Focke, P. Fortin, Y. Fukazawa, S. Funk, P. Fusco, F. Gargano, D. Gasparrini, N. Gehrels, S. Germani, N. Giglietto, F. Giordano, M. Giroletti, T. Glanzman, G. Godfrey, I. A. Grenier, J. E. Grove, S. Guiriec, D. Hadasch, Y. Hanabata, A. K. Harding, M. Hayashida, E. Hays, A. B. Hill, R. E. Hughes, G. Jóhannesson, A. S. Johnson, T. J. Johnson, T. Kamae, H. Katagiri, J. Kataoka, M. Kerr, J. Knödlseder, M. Kuss, J. Lande, F. Longo, F. Loparco, M. N. Lovellette, P. Lubrano, M. N. Mazziotta, J. E. McEnery, P. F. Michelson, W. Mitthumsiri, T. Mizuno, C. Monte, M. E. Monzani, A. Morselli, I. V. Moskalenko, S. Murgia, T. Nakamori, M. Naumann-Godo, J. P. Norris, E. Nuss, M. Ohno, T. Ohsugi, A. Okumura, N. Omodei, E. Orlando, M. Ozaki, D. Paneque, D. Parent, M. Pesce-Rollins, M. Pierbattista, F. Piron, G. Pivato, T. A. Porter, S. Rainò, R. Rando, M. Razzano, A. Reimer, O. Reimer, S. Ritz, R. W. Romani, M. Roth, P. M. Saz Parkinson, C. Sgrò, E. J. Siskind, G. Spandre, P. Spinelli, 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, T. L. Usher, J. Vandenbroucke, G. Vianello, V. Vitale, A. P. Waite, B. L. Winer, K. S. Wood, M. Wood, Z. Yang, S. Zimmer, M. J. Coe, F. Di Mille, P. G. Edwards, M. D. Filipović, J. L. Payne, J. Stevens, M. A.P. Torres

Stanford University
Universite Paris-Saclay
INFN Sezione di Trieste
University of Trieste
INFN
University of Padova
University of California at Santa Cruz
University of Pavia
INAF Istituto di Astrofisica Spaziale e Fisica Cosmica, Milan
Istituto Nazionale di Fisica Nucleare, Sezione di Pisa
INFN Sezione di Perugia
University of Perugia
Politecnico di Bari
INFN Sezione di Bari
University of Sheffield
Science and Research Directorate
NASA Goddard Space Flight Center
Biochemical and Environmental Engineering
Artep Inc.
Naval Research Laboratory
National Research Council
ASI Science Data Center
Laboratoire Univers et Particules de Montpellier
Institut Universitaire de France
Scuola Universitaria Superiore IUSS di Pavia
University of Maryland
Université Grenoble Alpes
Ip Paris
Hiroshima University
INAF Istituto di Radioastronomia
Center for Space Plasma and Aeronomic Research
Department of Astronomy, Graduate School of Science, Kyoto University
University of Southampton
The Ohio State University
University of Iceland
Ibaraki University
Waseda University
IRAP/CNRS
Université Paul Sabatier
INFN Roma Tor Vergata
Boise State University
ISAS/JAXA
Max Planck Institut für Extraterrestrische Physik
Max-Planck-Institut für Physik
George Mason University
Medical University of Innsbruck
University of Washington
NYCB Real-Time Computing Inc.
Purdue University Northwest
Pompeu Fabra University (UPF)
Consorzio Interuniversitario per la Fisica Spaziale (CIFS)
University of Rome “Tor Vergata”
Stockholm University
Oskar Klein Centre
Australian Astronomical Observatory-Las Campanas Observatory, Colina
Commonwealth Scientific and Industrial Research Organization
Western Sydney University
Center for Astrophysics | Harvard & Smithsonian

Résultats de recherche: Contribution à un journal › Article › Revue par des pairs

100 Citations (Scopus)

Résumé

Gamma-ray binaries are stellar systems containing a neutron star or black hole, with gamma-ray emission produced by an interaction between the components. These systems are rare, even though binary evolution models predict dozens in our Galaxy. A search for gamma-ray binaries with the Fermi Large Area Telescope (LAT) shows that 1FGL J1018.6-5856 exhibits intensity and spectral modulation with a 16.6-day period. We identified a variable x-ray counterpart, which shows a sharp maximum coinciding with maximum gamma-ray emission, as well as an O6V((f)) star optical counterpart and a radio counterpart that is also apparently modulated on the orbital period. 1FGL J1018.6-5856 is thus a gamma-ray binary, and its detection suggests the presence of other fainter binaries in the Galaxy.

langue originale	Anglais
Pages (de - à)	189-193
Nombre de pages	5
journal	Science
Volume	335
Numéro de publication	6065
Les DOIs	https://doi.org/10.1126/science.1213974
état	Publié - 13 janv. 2012

Accès au document

10.1126/science.1213974

Contient cette citation

Ackermann, M., Ajello, M., Ballet, J., Barbiellini, G., Bastieri, D., Belfiore, A., Bellazzini, R., Berenji, B., Blandford, R. D., Bloom, E. D., Bonamente, E., Borgland, A. W., Bregeon, J., Brigida, M., Bruel, P., Buehler, R., Buson, S., Caliandro, G. A., Cameron, R. A., ... Torres, M. A. P. (2012). Periodic emission from the gamma-ray binary 1FGL J1018.6-5856. Science, 335(6065), 189-193. https://doi.org/10.1126/science.1213974

@article{11bc06fbab5b49d79ab24c4480fa8945,

title = "Periodic emission from the gamma-ray binary 1FGL J1018.6-5856",

abstract = "Gamma-ray binaries are stellar systems containing a neutron star or black hole, with gamma-ray emission produced by an interaction between the components. These systems are rare, even though binary evolution models predict dozens in our Galaxy. A search for gamma-ray binaries with the Fermi Large Area Telescope (LAT) shows that 1FGL J1018.6-5856 exhibits intensity and spectral modulation with a 16.6-day period. We identified a variable x-ray counterpart, which shows a sharp maximum coinciding with maximum gamma-ray emission, as well as an O6V((f)) star optical counterpart and a radio counterpart that is also apparently modulated on the orbital period. 1FGL J1018.6-5856 is thus a gamma-ray binary, and its detection suggests the presence of other fainter binaries in the Galaxy.",

author = "M. Ackermann and M. Ajello and J. Ballet and G. Barbiellini and D. Bastieri and A. Belfiore and R. Bellazzini and B. Berenji and Blandford, \{R. D.\} and Bloom, \{E. D.\} and E. Bonamente and Borgland, \{A. W.\} and J. Bregeon and M. Brigida and P. Bruel and R. Buehler and S. Buson and Caliandro, \{G. A.\} and Cameron, \{R. A.\} and Caraveo, \{P. A.\} and E. Cavazzuti and C. Cecchi and {\"O} {\c C}elik and E. Charles and S. Chaty and A. Chekhtman and Cheung, \{C. C.\} and J. Chiang and S. Ciprini and R. Claus and J. Cohen-Tanugi and S. Corbel and Corbet, \{R. H.D.\} and S. Cutini and \{De Luca\}, A. and \{Den Hartog\}, \{P. R.\} and \{De Palma\}, F. and Dermer, \{C. D.\} and Digel, \{S. W.\} and \{Do Couto E Silva\}, E. and D. Donato and Drell, \{P. S.\} and A. Drlica-Wagner and R. Dubois and G. Dubus and C. Favuzzi and Fegan, \{S. J.\} and Ferrara, \{E. C.\} and Focke, \{W. B.\} and P. Fortin and Y. Fukazawa and S. Funk and P. Fusco and F. Gargano and D. Gasparrini and N. Gehrels 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 Y. Hanabata and Harding, \{A. K.\} and M. Hayashida and E. Hays and Hill, \{A. B.\} and Hughes, \{R. E.\} and G. J{\'o}hannesson and Johnson, \{A. S.\} and Johnson, \{T. J.\} and T. Kamae and H. Katagiri and J. Kataoka and M. Kerr and J. Kn{\"o}dlseder and M. Kuss and J. Lande and F. Longo and F. Loparco and Lovellette, \{M. N.\} and P. Lubrano and Mazziotta, \{M. N.\} and McEnery, \{J. E.\} and Michelson, \{P. F.\} and W. Mitthumsiri and T. Mizuno and C. Monte and Monzani, \{M. E.\} and A. Morselli and Moskalenko, \{I. V.\} and S. Murgia and T. Nakamori and M. Naumann-Godo and Norris, \{J. P.\} and E. Nuss and M. Ohno and T. Ohsugi and A. Okumura and N. Omodei and E. Orlando and M. Ozaki and D. Paneque and D. Parent and M. Pesce-Rollins and M. Pierbattista and F. Piron and G. Pivato and Porter, \{T. A.\} and S. Rain{\`o} and R. Rando and M. Razzano and A. Reimer and O. Reimer and S. Ritz and Romani, \{R. W.\} and M. Roth and \{Saz Parkinson\}, \{P. M.\} and C. Sgr{\`o} and Siskind, \{E. J.\} and G. Spandre and P. Spinelli 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 Usher, \{T. L.\} and J. Vandenbroucke and G. Vianello and V. Vitale and Waite, \{A. P.\} and Winer, \{B. L.\} and Wood, \{K. S.\} and M. Wood and Z. Yang and S. Zimmer and Coe, \{M. J.\} and \{Di Mille\}, F. and Edwards, \{P. G.\} and Filipovi{\'c}, \{M. D.\} and Payne, \{J. L.\} and J. Stevens and Torres, \{M. A.P.\}",

year = "2012",

month = jan,

day = "13",

doi = "10.1126/science.1213974",

language = "English",

volume = "335",

pages = "189--193",

journal = "Science",

issn = "0036-8075",

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

number = "6065",

}

Ackermann, M, Ajello, M, Ballet, J, Barbiellini, G, Bastieri, D, Belfiore, A, Bellazzini, R, Berenji, B, Blandford, RD, Bloom, ED, Bonamente, E, Borgland, AW, Bregeon, J, Brigida, M, Bruel, P, Buehler, R, Buson, S, Caliandro, GA, Cameron, RA, Caraveo, PA, Cavazzuti, E, Cecchi, C, Çelik, Ö, Charles, E, Chaty, S, Chekhtman, A, Cheung, CC, Chiang, J, Ciprini, S, Claus, R, Cohen-Tanugi, J, Corbel, S, Corbet, RHD, Cutini, S, De Luca, A, Den Hartog, PR, De Palma, F, Dermer, CD, Digel, SW, Do Couto E Silva, E, Donato, D, Drell, PS, Drlica-Wagner, A, Dubois, R, Dubus, G, Favuzzi, C, Fegan, SJ, Ferrara, EC, Focke, WB, Fortin, P, 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, IA, Grove, JE, Guiriec, S, Hadasch, D, Hanabata, Y, Harding, AK, Hayashida, M, Hays, E, Hill, AB, Hughes, RE, Jóhannesson, G, Johnson, AS, Johnson, TJ, Kamae, T, Katagiri, H, Kataoka, J, Kerr, M, Knödlseder, J, Kuss, M, Lande, J, Longo, F, Loparco, F, Lovellette, MN, Lubrano, P, Mazziotta, MN, McEnery, JE, Michelson, PF, Mitthumsiri, W, Mizuno, T, Monte, C, Monzani, ME, Morselli, A, Moskalenko, IV, Murgia, S, Nakamori, T, Naumann-Godo, M, Norris, JP, Nuss, E, Ohno, M, Ohsugi, T, Okumura, A, Omodei, N, Orlando, E, Ozaki, M, Paneque, D, Parent, D, Pesce-Rollins, M, Pierbattista, M, Piron, F, Pivato, G, Porter, TA, Rainò, S, Rando, R, Razzano, M, Reimer, A, Reimer, O, Ritz, S, Romani, RW, Roth, M, Saz Parkinson, PM, Sgrò, C, Siskind, EJ, Spandre, G, Spinelli, P, Suson, DJ, Takahashi, H, Tanaka, T, Thayer, JG, Thayer, JB, Thompson, DJ, Tibaldo, L, Tinivella, M, Torres, DF, Tosti, G, Troja, E, Uchiyama, Y, Usher, TL, Vandenbroucke, J, Vianello, G, Vitale, V, Waite, AP, Winer, BL, Wood, KS, Wood, M, Yang, Z, Zimmer, S, Coe, MJ, Di Mille, F, Edwards, PG, Filipović, MD, Payne, JL, Stevens, J & Torres, MAP 2012, 'Periodic emission from the gamma-ray binary 1FGL J1018.6-5856', Science, VOL. 335, Numéro 6065, p. 189-193. https://doi.org/10.1126/science.1213974

TY - JOUR

T1 - Periodic emission from the gamma-ray binary 1FGL J1018.6-5856

AU - Ackermann, M.

AU - Ajello, M.

AU - Ballet, J.

AU - Barbiellini, G.

AU - Bastieri, D.

AU - Belfiore, A.

AU - Bellazzini, R.

AU - Berenji, B.

AU - Blandford, R. D.

AU - Bloom, E. D.

AU - Bonamente, E.

AU - Borgland, A. W.

AU - Bregeon, J.

AU - Brigida, M.

AU - Bruel, P.

AU - Buehler, R.

AU - Buson, S.

AU - Caliandro, G. A.

AU - Cameron, R. A.

AU - Caraveo, P. A.

AU - Cavazzuti, E.

AU - Cecchi, C.

AU - Çelik, Ö

AU - Charles, E.

AU - Chaty, S.

AU - Chekhtman, A.

AU - Cheung, C. C.

AU - Chiang, J.

AU - Ciprini, S.

AU - Claus, R.

AU - Cohen-Tanugi, J.

AU - Corbel, S.

AU - Corbet, R. H.D.

AU - Cutini, S.

AU - De Luca, A.

AU - Den Hartog, P. R.

AU - De Palma, F.

AU - Dermer, C. D.

AU - Digel, S. W.

AU - Do Couto E Silva, E.

AU - Donato, D.

AU - Drell, P. S.

AU - Drlica-Wagner, A.

AU - Dubois, R.

AU - Dubus, G.

AU - Favuzzi, C.

AU - Fegan, S. J.

AU - Ferrara, E. C.

AU - Focke, W. B.

AU - Fortin, P.

AU - Fukazawa, Y.

AU - Funk, S.

AU - Fusco, P.

AU - Gargano, F.

AU - Gasparrini, D.

AU - Gehrels, N.

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 - Hanabata, Y.

AU - Harding, A. K.

AU - Hayashida, M.

AU - Hays, E.

AU - Hill, A. B.

AU - Hughes, R. E.

AU - Jóhannesson, G.

AU - Johnson, A. S.

AU - Johnson, T. J.

AU - Kamae, T.

AU - Katagiri, H.

AU - Kataoka, J.

AU - Kerr, M.

AU - Knödlseder, J.

AU - Kuss, M.

AU - Lande, J.

AU - Longo, F.

AU - Loparco, F.

AU - Lovellette, M. N.

AU - Lubrano, P.

AU - Mazziotta, M. N.

AU - McEnery, J. E.

AU - Michelson, P. F.

AU - Mitthumsiri, W.

AU - Mizuno, T.

AU - Monte, C.

AU - Monzani, M. E.

AU - Morselli, A.

AU - Moskalenko, I. V.

AU - Murgia, S.

AU - Nakamori, T.

AU - Naumann-Godo, M.

AU - Norris, J. P.

AU - Nuss, E.

AU - Ohno, M.

AU - Ohsugi, T.

AU - Okumura, A.

AU - Omodei, N.

AU - Orlando, E.

AU - Ozaki, M.

AU - Paneque, D.

AU - Parent, D.

AU - Pesce-Rollins, M.

AU - Pierbattista, M.

AU - Piron, F.

AU - Pivato, G.

AU - Porter, T. A.

AU - Rainò, S.

AU - Rando, R.

AU - Razzano, M.

AU - Reimer, A.

AU - Reimer, O.

AU - Ritz, S.

AU - Romani, R. W.

AU - Roth, M.

AU - Saz Parkinson, P. M.

AU - Sgrò, C.

AU - Siskind, E. J.

AU - Spandre, G.

AU - Spinelli, P.

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 - Usher, T. L.

AU - Vandenbroucke, J.

AU - Vianello, G.

AU - Vitale, V.

AU - Waite, A. P.

AU - Winer, B. L.

AU - Wood, K. S.

AU - Wood, M.

AU - Yang, Z.

AU - Zimmer, S.

AU - Coe, M. J.

AU - Di Mille, F.

AU - Edwards, P. G.

AU - Filipović, M. D.

AU - Payne, J. L.

AU - Stevens, J.

AU - Torres, M. A.P.

PY - 2012/1/13

Y1 - 2012/1/13

N2 - Gamma-ray binaries are stellar systems containing a neutron star or black hole, with gamma-ray emission produced by an interaction between the components. These systems are rare, even though binary evolution models predict dozens in our Galaxy. A search for gamma-ray binaries with the Fermi Large Area Telescope (LAT) shows that 1FGL J1018.6-5856 exhibits intensity and spectral modulation with a 16.6-day period. We identified a variable x-ray counterpart, which shows a sharp maximum coinciding with maximum gamma-ray emission, as well as an O6V((f)) star optical counterpart and a radio counterpart that is also apparently modulated on the orbital period. 1FGL J1018.6-5856 is thus a gamma-ray binary, and its detection suggests the presence of other fainter binaries in the Galaxy.

AB - Gamma-ray binaries are stellar systems containing a neutron star or black hole, with gamma-ray emission produced by an interaction between the components. These systems are rare, even though binary evolution models predict dozens in our Galaxy. A search for gamma-ray binaries with the Fermi Large Area Telescope (LAT) shows that 1FGL J1018.6-5856 exhibits intensity and spectral modulation with a 16.6-day period. We identified a variable x-ray counterpart, which shows a sharp maximum coinciding with maximum gamma-ray emission, as well as an O6V((f)) star optical counterpart and a radio counterpart that is also apparently modulated on the orbital period. 1FGL J1018.6-5856 is thus a gamma-ray binary, and its detection suggests the presence of other fainter binaries in the Galaxy.

U2 - 10.1126/science.1213974

DO - 10.1126/science.1213974

M3 - Article

AN - SCOPUS:84862908430

SN - 0036-8075

VL - 335

SP - 189

EP - 193

JO - Science

JF - Science

IS - 6065

ER -

Periodic emission from the gamma-ray binary 1FGL J1018.6-5856

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