2026-06-08T12:24:07Zhttps://docta.ucm.es/rest/oai/requestoai:docta.ucm.es:20.500.14352/508232024-09-05T18:29:50Zcom_20.500.14352_14col_20.500.14352_15
Docta Complutense
author
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
2023-06-20T10:37:41Z
2023-06-20T10:37:41Z
2008-09-20
2041-8205
10.1086/592433
https://hdl.handle.net/20.500.14352/50823
http://dx.doi.org/10.1086/592433
http://iopscience.iop.orghttp://arxiv.org/abs/0808.1832
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.
eng
First bounds on the high-energy emission from isolated Wolf-Rayet binary systems
journal article
URL
https://docta.ucm.es/bitstreams/cc512777-6618-44bb-bd88-a1a708d6f70e/download
File
MD5
a3978d33749590ec32cd8e7d9d9ce468
73372
application/pdf
MirandaJM53libre.pdf