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: | en_US |
| Published: |
IOP Publishing
2012
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| Online Access: | http://hdl.handle.net/1721.1/72092 |