Implications of X-ray Line Variations for 4u1822-371

4U 1822-371 is one of the prototype accretion disk coronal sources with an orbital period of about 5.6 hr. The binary is viewed almost edge-on at a high inclination angle of 83°, which makes it a unique candidate to study binary orbital and accretion disk dynamics in high powered X-ray sources. We o...

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Bibliographic Details
Main Authors: Schulz, Norbert S. (Contributor), Nowak, Michael A. (Contributor), Ji, Li (Author)
Other Authors: MIT Kavli Institute for Astrophysics and Space Research (Contributor), Canizares, Claude (Contributor), Ji, L. (Contributor)
Format: Article
Language:English
Published: IOP Publishing, 2012-08-10T13:48:17Z.
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