An X-ray Binary Model for the Galactic Center Source IRS 13E

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dc.creatorCoker, R. F.
dc.creatorPittard, J. M.
dc.date2000-08-04
dc.date.accessioned2026-07-07T01:54:41Z
dc.date.available2026-07-07T01:54:41Z
dc.descriptionWe present several models for IRS 13E, an infrared, mm and X-ray source in the Galactic Center. Our favored interpretation is that of an early-type binary with strong colliding winds emission. This naturally explains the observed X-ray count rate and the strong infrared emission lines, and has a distinct advantage over competing hypotheses based upon a single star or black-hole system.
dc.description5 pages, 3 figures, accepted by A&A Letters
dc.identifierhttps://arxiv.org/abs/astro-ph/0008091
dc.identifierhttp://arxiv.org/abs/astro-ph/0008091
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/1445
dc.subjectAstrophysics
dc.titleAn X-ray Binary Model for the Galactic Center Source IRS 13E
dc.typetext

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