AAS 207th Meeting, 8-12 January 2006
Session 183 Radio and X-Ray Pulsars
Poster, Thursday, 9:20am-4:00pm, January 12, 2006, Exhibit Hall

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[183.02] Evolution of the SAX J2103.5+4545 pulsar

M.J. Stark, C.M. Heffner (Lafayette College), A. Baykal (Middle East Technical University), J.H. Swank (NASA/Lab for High Energy Astrophysics)

Having precise phase-connected pulse timing data covering several years from SAX J2103.5+4545 and having constructed a precise orbital model, we turn to the careful analysis of the evolution of the pulsar. We present a study of the dependence of the derivative of the pulsar signal on the accretion rate for this source. This study is detailed enough to constrain several parameters of this system.


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The author(s) of this abstract have provided an email address for comments about the abstract: starkm@lafayette.edu

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