2003/01/29 by Christopher W. Mauche, Mauche, Christopher W.
Physics and Astronomy · #Astrophysics (astro-ph) #FOS: Physical sciences #astro-ph
paper · pdf · doi:10.48550/arxiv.astro-ph/0301582
4 pages including 3 encapsulated postscript figures; LaTeX format, uses newpasp.sty; to appear in the ASP Conference Series "IAU Colloquium No. 190--Magnetic Cataclysmic Variables"
arxiv created 2003/01/29 · arxiv updated 2009/12/01
We use hard X-ray light curves measured by the Chandra HETG and RXTE PCA during the late rise and plateau phases of the 2002 March-April outburst of the intermediate polar GK Per to determine that its X-ray pulse period P = 351.332 +/- 0.002 s. Combined with previous X-ray and optical measurements of the spin period of the white dwarf, we find that its spin-up rate Pdot = 0.00027 +/- 0.00005 s/yr.