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Bozzo+10 APACrefauthors Bozzo , E · 2010 · DOI 10.1051/0004-6361/201014095

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astro-ph.HE 1

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2024 1

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CONDITIONAL 1

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The role of XMM-Newton in the investigation of persistent BeXRBs

astro-ph.HE · 2024-11-22 · conditional · novelty 4.0

Persistent Be X-ray binaries share a hot (1-2 keV) blackbody component contributing 20-40% of the X-ray flux, with an emitting size close to the neutron star polar cap, and a new XMM-Newton observation of 4U 0728-25 fits this pattern.

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  • The role of XMM-Newton in the investigation of persistent BeXRBs astro-ph.HE · 2024-11-22 · conditional · none · ref 3

    Persistent Be X-ray binaries share a hot (1-2 keV) blackbody component contributing 20-40% of the X-ray flux, with an emitting size close to the neutron star polar cap, and a new XMM-Newton observation of 4U 0728-25 fits this pattern.