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.
|Titolo:||First Bounds on the High-Energy Emission from Isolated Wolf-Rayet Binary Systems|
|Citazione:||E., A., H., A., L. A., A., P., A., M., B., C., B., et al. (2008). First Bounds on the High-Energy Emission from Isolated Wolf-Rayet Binary Systems. THE ASTROPHYSICAL JOURNAL LETTERS, 685(1), L71-L74.|
|Appare nelle tipologie:||1.1 Articolo in rivista|
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