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...
Main Authors: | , , |
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Other Authors: | , , |
Format: | Article |
Language: | English |
Published: |
IOP Publishing,
2012-08-10T13:48:17Z.
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Subjects: | |
Online Access: | Get fulltext |