X-Ray Bursters A1742-294 and SLX1744-299/300 Near the Galactic Center

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dc.creatorLutovinov, A. A.
dc.creatorGrebenev, S. A.
dc.creatorPavlinsky, M. N.
dc.creatorSunyaev, R. A.
dc.date2000-09-21
dc.date.accessioned2026-07-07T01:55:34Z
dc.date.available2026-07-07T01:55:34Z
dc.descriptionWe present a study of two X-ray bursters in the Galactic Center field with the ART-P telescope onboard GRANAT. During 1990-1992 approximately 100 X-ray bursts were detected from the Galactic Center field and most of them were identified with the two persistent sources, A1742-294 and SLX1744-299/300. The burst recurrence times were found to be ~2.4 and ~4.6 hours, respectively, which is significantly shorter them was previously thought. We calculated the mean and maximum fluxes during the bursts and investigated their time profiles. We found that the shape of A1742-294 bursts correlates with the burst peak flux. The spectral analysis was carried out for the strongest burst, detected from A1742-294 on Oct 18, 1990.
dc.description7 pages (5 figures), to be published in the proceedings of ``X-Ray Astronomy 2000'', Palermo, Italy
dc.identifierhttps://arxiv.org/abs/astro-ph/0009349
dc.identifierhttp://arxiv.org/abs/astro-ph/0009349
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/1702
dc.subjectAstrophysics
dc.titleX-Ray Bursters A1742-294 and SLX1744-299/300 Near the Galactic Center
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