Pulse-to-pulse variations in accreting X-ray pulsars

In most accreting X-ray pulsars, the periodic signal is very clear and easily shows up as soon as data covering sufficient pulse periods (a few ten) are available. The mean pulse profile is often quite typical for a given source and with minor variations repeated and recognisable across observations...

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Bibliografiske detaljer

Principais autores:	Kretschmar Peter, Marcu Diana, Kühnel Matthias, Klochkov Dmitry, Pottschmidt Katja, Staubert Rüdiger, Wilson-Hodge Colleen A., Jenke Peter A., Caballero Isabel, Fürst Felix
Format:	Artigo
Sprog:	Inglês
Udgivet:	EDP Sciences 2014-01-01
Serier:	EPJ Web of Conferences
Online adgang:	http://dx.doi.org/10.1051/epjconf/20136406012
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