THE SPECTRAL EVOLUTION ALONG THE Z TRACK OF THE BRIGHT NEUTRON STAR X-RAY BINARY GX 17+2

Z sources are bright neutron star X-ray binaries, accreting at around the Eddington limit. We analyze the 68 RXTE observations (~270 ks) of Sco-like Z source GX 17+2 made between 1999 October 3 and 12, covering a complete Z track. We create and fit color-resolved spectra with a model consisting of a...

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Bibliographic Details
Main Authors: Lin, Dacheng (Author), Homan, Jeroen (Contributor), Barret, Didier (Author), Remillard, Ronald A (Author)
Other Authors: MIT Kavli Institute for Astrophysics and Space Research (Contributor), Remillard, Ronald Alan (Contributor)
Format: Article
Language:English
Published: IOP Publishing, 2015-02-25T18:45:17Z.
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