Thermonuclear burning in the matter accumulated on the surface of an accreting neutron star is unstable under certain conditions, which leads to powerful explosions also called Type I X-ray bursts. This book covers the theory of spectral formation in the atmospheres of neutron stars during these violent events as well as its application to observational data on X-ray bursts. The main goal of the presented study is a proper measurement of the fundamental properties for neutron stars. We take both analytical and numerical approaches to the problem of radiative transfer in X-ray illuminated atmospheres which account for all crucial physical factors such as Comptonization, free-free absorption and emission. We apply our models to the data collected with NASA's Rossi X-ray Timing Explorer mission in order to constrain neutron star masses and radii for five X-ray burster 4U 1728-34, 4U 1820-30, Cygnus X-2, EXO 0748-676 and GS 1826-24. The developed neutron star mass-radius measurement method has a great potential for application to new and archival X-ray data. It can provide scientists with a vital information on various aspects of physics of compact objects.
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Etat : New. Thermonuclear burning in the matter accumulatedon the surface of an accreting neutron star isunstable under certain conditions, which leads topowerful explosions also called Type I X-raybursts. This book covers the theory ofspectral formation in the atmosph. N° de réf. du vendeur 4954489
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Taschenbuch. Etat : Neu. Neuware - Thermonuclear burning in the matter accumulatedon the surface of an accreting neutron star isunstable under certain conditions, which leads topowerful explosions also called Type I X-raybursts. This book covers the theory ofspectral formation in the atmospheres of neutronstars during these violent events as well as itsapplication to observational data on X-ray bursts.The main goal of the presented study is a propermeasurement of the fundamental properties forneutron stars. We take bothanalytical and numerical approaches to the problem ofradiative transfer in X-ray illuminated atmosphereswhich account for all crucial physical factors suchas Comptonization, free-free absorption and emission.We apply our models to the data collected with NASA'sRossi X-ray Timing Explorer mission in order toconstrain neutron star masses and radii for fiveX-ray burster 4U 1728-34, 4U 1820-30, Cygnus X-2, EXO0748-676 and GS 1826-24. The developed neutron starmass-radius measurement method has a great potentialfor application to new and archival X-ray data. Itcan provide scientists with a vital information onvarious aspects of physics of compact objects. N° de réf. du vendeur 9783639068887
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