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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.

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 [10.1086/592433].

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

BONNOLI, GIACOMO;STAMERRA, ANTONIO;TURINI, NICOLA;
2008-01-01

Abstract

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.
2008
THE ASTROPHYSICAL JOURNAL LETTERS
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 [10.1086/592433].
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11365/44467
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