First bounds on the high-energy emission from isolated Wolf-Rayet binary systems

E. Aliu; H. Anderhub; L. A. Antonelli; P. Antoranz; M. Backes; C. Baixeras; J. A. Barrio; H. Bartko; D. Bastieri; J. K. Becker; W. Bednarek; K. Berger; E. Bernardini; C. Bigongiari; A. Biland; R. K. Bock; G. Bonnoli; P. Bordas; V. Bosch-Ramon; T. Bretz; I. Britvitch; M. Camara; E. Carmona; A. Chilingarian; S. Commichau; J. L. Contreras; J. Cortina; M. T. Costado; S. Covino; V. Curtef; F. Dazzi; A. De Angelis; E. De Cea del Pozo; R. De Los Reyes; B. De Lotto; M. De Maria; F. De Sabata; C. Delgado Mendez; A. Dominguez; D. Dorner; M. Doro; M. Errando; M. Fagiolini; D. Ferenc; E. Fernández; R. Firpo; M. V. Fonseca; L. Font; N. Galante; R. J. Garcýa López; M. Garczarczyk; M. Gaug; F. Goebel; M. Hayashida; A. Herrero; D. Höhne; J. Hose; C. C. Hsu; S. Huber; T. Jogler; D. Kranich; A. La Barbera; A. Laille; E. Leonardo; E. Lindfors; S. Lombardi; F. Longo; M. López; E. Lorenz; P. Majumdar; G. Maneva; N. Mankuzhiyil; K. Mannheim; L. Maraschi; M. Mariotti; M. Martýnez; D. Mazin; M. Meucci; M. Meyer; J. M. Miranda; R. Mirzoyan; M. Moles; A. Moralejo; D. Nieto; K. Nilsson; J. Ninkovic; E. Oña-Wilhelmi; N. Otte; I. Oya; R. Paoletti; J. M. Paredes; M. Pasanen; D. Pascoli; F. Pauss; R. G. Pegna; M. A. Perez-Torres; M. Persic; L. Peruzzo; A. Piccioli; F. Prada

doi:10.1086/592433

First bounds on the high-energy emission from isolated Wolf-Rayet binary systems

E. Aliu, H. Anderhub, L. A. Antonelli, P. Antoranz, M. Backes, C. Baixeras, J. A. Barrio, H. Bartko, D. Bastieri, J. K. Becker, W. Bednarek, K. Berger, E. Bernardini, C. Bigongiari, A. Biland, R. K. Bock, G. Bonnoli, P. Bordas, V. Bosch-Ramon, T. BretzI. Britvitch, M. Camara, E. Carmona, A. Chilingarian, S. Commichau, J. L. Contreras, J. Cortina, M. T. Costado, S. Covino, V. Curtef, F. Dazzi, A. De Angelis, E. De Cea del Pozo, R. De Los Reyes, B. De Lotto, M. De Maria, F. De Sabata, C. Delgado Mendez, A. Dominguez, D. Dorner, M. Doro, M. Errando, M. Fagiolini, D. Ferenc, E. Fernández, R. Firpo, M. V. Fonseca, L. Font, N. Galante, R. J. Garcýa López, M. Garczarczyk, M. Gaug, F. Goebel, M. Hayashida, A. Herrero, D. Höhne, J. Hose, C. C. Hsu, S. Huber, T. Jogler, D. Kranich, A. La Barbera, A. Laille, E. Leonardo, E. Lindfors, S. Lombardi, F. Longo, M. López, E. Lorenz, P. Majumdar, G. Maneva, N. Mankuzhiyil, K. Mannheim, L. Maraschi, M. Mariotti, M. Martýnez, D. Mazin, M. Meucci, M. Meyer, J. M. Miranda, R. Mirzoyan, M. Moles, A. Moralejo, D. Nieto, K. Nilsson, J. Ninkovic, E. Oña-Wilhelmi, N. Otte, I. Oya, R. Paoletti, J. M. Paredes, M. Pasanen, D. Pascoli, F. Pauss, R. G. Pegna, M. A. Perez-Torres, M. Persic, L. Peruzzo, A. Piccioli, F. Prada

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Resum

High-energy gamma-ray emission is theoretically expected to arise in tight binary star systems (with high mass loss and high-velocity winds), although the evidence of this relationship has proven to be elusive so far. Here we present the first bounds on this putative emission from isolated Wolf-Rayet (WR) star binaries, WR 147 and WR 146, obtained from observations with the MAGIC telescope. © 2008. The American Astronomical Society. All rights reserved.

Idioma original	Anglès
Revista	Astrophysical Journal
Volum	685
Número	1 PART 2
DOIs	https://doi.org/10.1086/592433
Estat de la publicació	Publicada - 1 de gen. 2008

Accés al document

10.1086/592433

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https://www.scopus.com/pages/publications/65549153582

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Aliu, E., Anderhub, H., Antonelli, L. A., Antoranz, P., Backes, M., Baixeras, C., Barrio, J. A., Bartko, H., Bastieri, D., Becker, J. K., Bednarek, W., Berger, K., Bernardini, E., Bigongiari, C., Biland, A., Bock, R. K., Bonnoli, G., Bordas, P., Bosch-Ramon, V., ... Prada, F. (2008). First bounds on the high-energy emission from isolated Wolf-Rayet binary systems. Astrophysical Journal, 685(1 PART 2). https://doi.org/10.1086/592433

@article{1dfc5850549048918d4f52d42dfdeedb,

title = "First bounds on the high-energy emission from isolated Wolf-Rayet binary systems",

abstract = "High-energy gamma-ray emission is theoretically expected to arise in tight binary star systems (with high mass loss and high-velocity winds), although the evidence of this relationship has proven to be elusive so far. Here we present the first bounds on this putative emission from isolated Wolf-Rayet (WR) star binaries, WR 147 and WR 146, obtained from observations with the MAGIC telescope. {\textcopyright} 2008. The American Astronomical Society. All rights reserved.",

keywords = "Gamma rays, Observations, Subject heading",

author = "E. Aliu and H. Anderhub and Antonelli, \{L. A.\} and P. Antoranz and M. Backes and C. Baixeras and Barrio, \{J. A.\} and H. Bartko and D. Bastieri and Becker, \{J. K.\} and W. Bednarek and K. Berger and E. Bernardini and C. Bigongiari and A. Biland and Bock, \{R. K.\} and G. Bonnoli and P. Bordas and V. Bosch-Ramon and T. Bretz and I. Britvitch and M. Camara and E. Carmona and A. Chilingarian and S. Commichau and Contreras, \{J. L.\} and J. Cortina and Costado, \{M. T.\} and S. Covino and V. Curtef and F. Dazzi and \{De Angelis\}, A. and \{De Cea del Pozo\}, E. and \{De Los Reyes\}, R. and \{De Lotto\}, B. and \{De Maria\}, M. and \{De Sabata\}, F. and \{Delgado Mendez\}, C. and A. Dominguez and D. Dorner and M. Doro and M. Errando and M. Fagiolini and D. Ferenc and E. Fern{\'a}ndez and R. Firpo and Fonseca, \{M. V.\} and L. Font and N. Galante and \{Garc{\'y}a L{\'o}pez\}, \{R. J.\} and M. Garczarczyk and M. Gaug and F. Goebel and M. Hayashida and A. Herrero and D. H{\"o}hne and J. Hose and Hsu, \{C. C.\} and S. Huber and T. Jogler and D. Kranich and \{La Barbera\}, A. and A. Laille and E. Leonardo and E. Lindfors and S. Lombardi and F. Longo and M. L{\'o}pez and E. Lorenz and P. Majumdar and G. Maneva and N. Mankuzhiyil and K. Mannheim and L. Maraschi and M. Mariotti and M. Mart{\'y}nez and D. Mazin and M. Meucci and M. Meyer and Miranda, \{J. M.\} and R. Mirzoyan and M. Moles and A. Moralejo and D. Nieto and K. Nilsson and J. Ninkovic and E. O{\~n}a-Wilhelmi and N. Otte and I. Oya and R. Paoletti and Paredes, \{J. M.\} and M. Pasanen and D. Pascoli and F. Pauss and Pegna, \{R. G.\} and Perez-Torres, \{M. A.\} and M. Persic and L. Peruzzo and A. Piccioli and F. Prada",

year = "2008",

month = jan,

day = "1",

doi = "10.1086/592433",

language = "English",

volume = "685",

journal = "Astrophysical Journal",

issn = "0004-637X",

publisher = "American Astronomical Society",

number = "1 PART 2",

}

Aliu, E, Anderhub, H, Antonelli, LA, Antoranz, P, Backes, M, Baixeras, C, Barrio, JA, Bartko, H, Bastieri, D, Becker, JK, Bednarek, W, Berger, K, Bernardini, E, Bigongiari, C, Biland, A, Bock, RK, Bonnoli, G, Bordas, P, Bosch-Ramon, V, Bretz, T, Britvitch, I, Camara, M, Carmona, E, Chilingarian, A, Commichau, S, Contreras, JL, Cortina, J, Costado, MT, Covino, S, Curtef, V, Dazzi, F, De Angelis, A, De Cea del Pozo, E, De Los Reyes, R, De Lotto, B, De Maria, M, De Sabata, F, Delgado Mendez, C, Dominguez, A, Dorner, D, Doro, M, Errando, M, Fagiolini, M, Ferenc, D, Fernández, E, Firpo, R, Fonseca, MV, Font, L, Galante, N, Garcýa López, RJ, Garczarczyk, M, Gaug, M, Goebel, F, Hayashida, M, Herrero, A, Höhne, D, Hose, J, Hsu, CC, Huber, S, Jogler, T, Kranich, D, La Barbera, A, Laille, A, Leonardo, E, Lindfors, E, Lombardi, S, Longo, F, López, M, Lorenz, E, Majumdar, P, Maneva, G, Mankuzhiyil, N, Mannheim, K, Maraschi, L, Mariotti, M, Martýnez, M, Mazin, D, Meucci, M, Meyer, M, Miranda, JM, Mirzoyan, R, Moles, M, Moralejo, A, Nieto, D, Nilsson, K, Ninkovic, J, Oña-Wilhelmi, E, Otte, N, Oya, I, Paoletti, R, Paredes, JM, Pasanen, M, Pascoli, D, Pauss, F, Pegna, RG, Perez-Torres, MA, Persic, M, Peruzzo, L, Piccioli, A & Prada, F 2008, 'First bounds on the high-energy emission from isolated Wolf-Rayet binary systems', Astrophysical Journal, vol. 685, núm. 1 PART 2. https://doi.org/10.1086/592433

TY - JOUR

T1 - First bounds on the high-energy emission from isolated Wolf-Rayet binary systems

AU - Aliu, E.

AU - Anderhub, H.

AU - Antonelli, L. A.

AU - Antoranz, P.

AU - Backes, M.

AU - Baixeras, C.

AU - Barrio, J. A.

AU - Bartko, H.

AU - Bastieri, D.

AU - Becker, J. K.

AU - Bednarek, W.

AU - Berger, K.

AU - Bernardini, E.

AU - Bigongiari, C.

AU - Biland, A.

AU - Bock, R. K.

AU - Bonnoli, G.

AU - Bordas, P.

AU - Bosch-Ramon, V.

AU - Bretz, T.

AU - Britvitch, I.

AU - Camara, M.

AU - Carmona, E.

AU - Chilingarian, A.

AU - Commichau, S.

AU - Contreras, J. L.

AU - Cortina, J.

AU - Costado, M. T.

AU - Covino, S.

AU - Curtef, V.

AU - Dazzi, F.

AU - De Angelis, A.

AU - De Cea del Pozo, E.

AU - De Los Reyes, R.

AU - De Lotto, B.

AU - De Maria, M.

AU - De Sabata, F.

AU - Delgado Mendez, C.

AU - Dominguez, A.

AU - Dorner, D.

AU - Doro, M.

AU - Errando, M.

AU - Fagiolini, M.

AU - Ferenc, D.

AU - Fernández, E.

AU - Firpo, R.

AU - Fonseca, M. V.

AU - Font, L.

AU - Galante, N.

AU - Garcýa López, R. J.

AU - Garczarczyk, M.

AU - Gaug, M.

AU - Goebel, F.

AU - Hayashida, M.

AU - Herrero, A.

AU - Höhne, D.

AU - Hose, J.

AU - Hsu, C. C.

AU - Huber, S.

AU - Jogler, T.

AU - Kranich, D.

AU - La Barbera, A.

AU - Laille, A.

AU - Leonardo, E.

AU - Lindfors, E.

AU - Lombardi, S.

AU - Longo, F.

AU - López, M.

AU - Lorenz, E.

AU - Majumdar, P.

AU - Maneva, G.

AU - Mankuzhiyil, N.

AU - Mannheim, K.

AU - Maraschi, L.

AU - Mariotti, M.

AU - Martýnez, M.

AU - Mazin, D.

AU - Meucci, M.

AU - Meyer, M.

AU - Miranda, J. M.

AU - Mirzoyan, R.

AU - Moles, M.

AU - Moralejo, A.

AU - Nieto, D.

AU - Nilsson, K.

AU - Ninkovic, J.

AU - Oña-Wilhelmi, E.

AU - Otte, N.

AU - Oya, I.

AU - Paoletti, R.

AU - Paredes, J. M.

AU - Pasanen, M.

AU - Pascoli, D.

AU - Pauss, F.

AU - Pegna, R. G.

AU - Perez-Torres, M. A.

AU - Persic, M.

AU - Peruzzo, L.

AU - Piccioli, A.

AU - Prada, F.

PY - 2008/1/1

Y1 - 2008/1/1

N2 - High-energy gamma-ray emission is theoretically expected to arise in tight binary star systems (with high mass loss and high-velocity winds), although the evidence of this relationship has proven to be elusive so far. Here we present the first bounds on this putative emission from isolated Wolf-Rayet (WR) star binaries, WR 147 and WR 146, obtained from observations with the MAGIC telescope. © 2008. The American Astronomical Society. All rights reserved.

AB - High-energy gamma-ray emission is theoretically expected to arise in tight binary star systems (with high mass loss and high-velocity winds), although the evidence of this relationship has proven to be elusive so far. Here we present the first bounds on this putative emission from isolated Wolf-Rayet (WR) star binaries, WR 147 and WR 146, obtained from observations with the MAGIC telescope. © 2008. The American Astronomical Society. All rights reserved.

KW - Gamma rays

KW - Observations

KW - Subject heading

UR - https://www.scopus.com/pages/publications/65549153582

U2 - 10.1086/592433

DO - 10.1086/592433

M3 - Article

SN - 0004-637X

VL - 685

JO - Astrophysical Journal

JF - Astrophysical Journal

IS - 1 PART 2

ER -

First bounds on the high-energy emission from isolated Wolf-Rayet binary systems

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