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.

If you would like more information about this abstract, please follow the link to http://www.lafayette.edu/~starkm/pub/aas-207.html. This link was provided by the author. When you follow it, you will leave the Web site for this meeting; to return, you should use the Back comand on your browser.

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

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