По вашему запросу найдено документов: 1120
Страница 1 из 112
Dynamo generated magnetic configurations in accretion discs and the nature of quasi-periodic oscillations in accreting binary systems© ESO 2016.Context. Magnetic fields are important for accretion disc structure. Magnetic fields
X-ray variability of ss 433: Effects of the supercritical accretion disc-correlation functions and power spectra depend drastically on the precession phase of the supercritical accretion disc
Dynamo generated magnetic configurations in accretion discs and the nature of quasi-periodic oscillations in accreting binary systems© ESO 2016.Context. Magnetic fields are important for accretion disc structure. Magnetic fields
Ultraluminous X-ray sources as neutrino pulsars. The classical limit on the accretion luminosity of a neutron star is given by the Eddington luminosity
Propeller effect in action in the ultraluminous accreting magnetar M82 X-2 in an accreting neutron star in binary System-The first pulsating ultraluminous X-Ray source X-2 in the galaxy M82
Evolution of broad-band SED during outburst rise in NS X-ray Nova Aql X-1 in 2013 can be understood in the framework of thermal emission from non-stationary accretion disc
Back reaction of the gravitational radiation on the metric of spacetime to the disappearance of the visible accretion disc of the merged pair of black holes.
Accreting millisecond pulsar SAX J1808.4-3658 during its 2002 outburst: Evidence for a receding discAn outburst of the accreting X-ray millisecond pulsar SAX J1808.4-3658 in 2002 October
X-ray variability of ss 433: Effects of the supercritical accretion disc-correlation functions and power spectra depend drastically on the precession phase of the supercritical accretion disc
Influence of rotation velocity gradient on line profiles of accretion discs of CVs discs. The complete disc structure is taken into account. The radial disc structure follows the alpha
Страница 1 из 112
Фасеты
Партнеры
Индексация
