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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.

FIRST BOUNDS ON THE HIGH-ENERGY EMISSION FROM ISOLATED WOLF-RAYET BINARY SYSTEMS RID B-5372-2009

SHORE, STEVEN NEIL;
2008-01-01

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.
2008
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; del Pozo, Ed; Reyes, Rd; De Lotto, B; De Maria, M; De Sabata, F; Mendez, Cd; Dominguez, A; Dorner, D; Doro, M; Errando, M; Fagiolini, M; Ferenc, D; Fernandez, E; Firpo, R; Fonseca, Mv; Font, L; Galante, N; Lopez, Rjg; Garczarczyk, M; Gaug, M; Goebel, F; Hayashida, M; Herrero, A; Hohne, D; Hose, J; Hsu, Cc; Huber, S; Jogler, T; Kranich, D; La Barbera, A; Laille, A; Leonardo, E; Lindfors, E; Lombardi, S; Longo, F; Lopez, M; Lorenz, E; Majumdar, P; Maneva, G; Mankuzhiyil, N; Mannheim, K; Maraschi, L; Mariotti, M; Martinez, M; Mazin, D; Meucci, M; Meyer, M; Miranda, Jm; Mirzoyan, R; Moles, M; Moralejo, A; Nieto, D; Nilsson, K; Ninkovic, J; Ona 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; Prandini, E; Puchades, N; Raymers, A; Rhode, W; Ribo, M; Rico, J; Rissi, M; Robert, A; Rugamer, S; Saggion, A; Saito, Ty; Salvati, M; Sanchez Conde, M; Sartori, P; Satalecka, K; Scalzotto, V; Scapin, V; Schweizer, T; Shayduk, M; Shinozaki, K; Shore, STEVEN NEIL; Sidro, N; Sierpowska Bartosik, A; Sillanpaa, A; Sobczynska, D; Spanier, F; Stamerra, A; Stark, Ls; Takalo, L; Tavecchio, F; Temnikov, P; Tescaro, D; Teshima, M; Tluczykont, M; Torres, Df; Turini, N; Vankov, H; Venturini, A; Vitale, V; Wagner, Rm; Wittek, W; Zabalza, V; Zandanel, F; Zanin, R; Zapatero, J.
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11568/125242
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