TY  - JOUR
AU  - Antoranz Canales, Pedro
AU  - Barrio Uña, Juan Abel
AU  - Contreras González, José Luis
AU  - Fonseca González, María Victoria
AU  - Miranda Pantoja, José Miguel
AU  - Nieto Castaño, Daniel
PY  - 2008
DO  - 10.1086/592433
SN  - 2041-8205
UR  - https://hdl.handle.net/20.500.14352/50823
T2  - Astrophysical journal letters
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...
LA  - eng
M2  - L71
PB  - IOP Publishing
KW  - Colliding-Wind Binary
KW  - Source TEV J2032+4130
KW  - X-Ray
KW  - Gamma-Rays
KW  - Follow-Up
KW  - WR 146
KW  - Radio
KW  - WR-147
KW  - LS-I-+61-303
KW  - Parameters.
TI  - First bounds on the high-energy emission from isolated Wolf-Rayet binary systems
TY  - journal article
VL  - 685
ER  -