SAX J1810.8-2609: an X-ray bursting transient

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dc.creatorCocchi, M.
dc.creatorBazzano, A.
dc.creatorNatalucci, L.
dc.creatorUbertini, P.
dc.creatorHeise, J.
dc.creatorMuller, J. M.
dc.creatorSmith, M. J. S.
dc.creatorZand, J. J. M. in 't
dc.date1999-01-18
dc.date.accessioned2026-07-07T02:30:01Z
dc.date.available2026-07-07T02:30:01Z
dc.descriptionWe report on the BeppoSAX/WFC observation of a strong type-I X-ray burst from the recently discovered transient source SAX J1810.8-2609. The observed event showed evidence of photospheric radius expansion due to super-Eddington burst luminosity. Burst detection identifies the source as a probable low-mass X-ray binary harbouring a neutron star.
dc.description4 pages, 3 figures, proc. 3rd INTEGRAL Workshop - Taormina 1998
dc.identifierhttps://arxiv.org/abs/astro-ph/9901230
dc.identifierhttp://arxiv.org/abs/astro-ph/9901230
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/13697
dc.subjectAstrophysics
dc.titleSAX J1810.8-2609: an X-ray bursting transient
dc.typetext

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