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dc.contributor.authorPiro, Luigi
dc.contributor.authorDe Pasquale, Massımılıano
dc.contributor.authorCosta, Enrico
dc.contributor.authorSoffitta, Paolo
dc.date.accessioned2021-03-05T10:24:21Z
dc.date.available2021-03-05T10:24:21Z
dc.identifier.citationSoffitta P., De Pasquale M., Piro L., Costa E., "The transition between the main event and the afterglow: BeppoSAX", 3rd Workshop on Gamma-Ray Bursts, Rome, İtalya, 17 - 20 Eylül 2002, cilt.312, ss.23-28
dc.identifier.othervv_1032021
dc.identifier.otherav_a2ea1f1a-984a-46fa-b2c2-d35d61cbac0e
dc.identifier.urihttp://hdl.handle.net/20.500.12627/109063
dc.description.abstractOne of the two Wide Field Cameras (WFCs) on board BeppoSAX was pointed towards the burst position for few orbits after the detection of the X-ray counterpart of the Gamma Ray Burst (GRB) till the repointing of Narrow Field Instruments (NFI). Therefore the WFC can provide a piece of knowledge on the different types of the transition between the main event and the afterglow. Results on a sub-samples of bursts show that the transition between the main event and the afterglow can be either smooth or can present gaps. In other cases the WFC data strongly suggest that a break should occur in the back extrapolation of the afterglow lightcurve detected by the NFI, nevertheless they do not rule-out a possible late appearing of the afterglow.
dc.language.isoeng
dc.subjectTemel Bilimler
dc.subjectFizik
dc.subjectAstronomi ve Astrofizik
dc.subjectTemel Bilimler (SCI)
dc.subjectUzay bilimi
dc.subjectASTRONOMİ VE ASTROFİZİK
dc.titleThe transition between the main event and the afterglow: BeppoSAX
dc.typeBildiri
dc.contributor.department, ,
dc.identifier.volume312
dc.contributor.firstauthorID103345


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