# name
First Bounds on the High-Energy Emission from Isolated Wolf-Rayet Binary Systems

# metadata.dc.description.abstract[].value
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.

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Astrophysical Journal Letters, 2008, vol. 685, num. 1, p. 71-74

# metadata.dc.source[].value
Articles publicats en revistes (Física Quàntica i Astrofísica)

# metadata.dc.title[].value
First Bounds on the High-Energy Emission from Isolated Wolf-Rayet Binary Systems