Registration of the First Thermonuclear X-ray Burst from AX J1754.2-2754

dc.creatorChelovekov, I. V.
dc.creatorGrebenev, S. A.
dc.date2007-10-30
dc.date.accessioned2026-07-07T11:38:25Z
dc.date.available2026-07-07T11:38:25Z
dc.descriptionDuring the analysis of the INTEGRAL observatory archival data we found a powerful X-ray burst, registered by JEM-X and IBIS/ISGRI telescopes on April 16, 2005 from a weak and poorly known source AX J1754.2-2754. Analysis of the burst profiles and spectrum shows, that it was a type I burst, which result from thermonuclear explosion on the surface of nutron star. It means that we can consider AX J1754.2-2754 as an X-ray burster. Certain features of burst profile at its initial stage witness of a radiation presure driven strong expansion and a corresponding cooling of the nutron star photosphere. Assuming, that the luminosity of the source at this phase was close to the Eddington limit, we estimated the distance to the burst source d=6.6+/-0.3 kpc (for hidrogen atmosphere of the neutron star) and d=9.2+/-0.4 kpc (for helium atmosphere).
dc.description12 pages, 6 figures
dc.identifierhttps://arxiv.org/abs/0710.5597
dc.identifierhttp://arxiv.org/abs/0710.5597
dc.identifierAstron.Lett.33:807-813,2007
dc.identifierdoi:10.1134/S1063773707120043
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/199559
dc.subjectAstrophysics
dc.titleRegistration of the First Thermonuclear X-ray Burst from AX J1754.2-2754
dc.typetext

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