2026-06-08T12:24:58Zhttps://docta.ucm.es/rest/oai/request

oai:docta.ucm.es:20.500.14352/508232024-09-05T18:29:50Zcom_20.500.14352_14col_20.500.14352_15

00925njm 22002777a 4500 dc Antoranz Canales, Pedro author Barrio Uña, Juan Abel author Contreras González, José Luis author Fonseca González, María Victoria author Miranda Pantoja, José Miguel author Nieto Castaño, Daniel author 2008-09-20 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. 2041-8205 10.1086/592433 https://hdl.handle.net/20.500.14352/50823 http://dx.doi.org/10.1086/592433 http://iopscience.iop.org http://arxiv.org/abs/0808.1832 First bounds on the high-energy emission from isolated Wolf-Rayet binary systems