IMPLICATIONS OF X-RAY LINE VARIATIONS FOR 4U1822–371
نویسندگان
چکیده
منابع مشابه
Implications of X-ray Line Variations for 4u1822−371
4U 1822−371 is one of the proto-type accretion disk coronal sources with an orbital period of about 5.6 hours. The binary is viewed almost edge-on at a high inclination angle of 83 degrees, which makes it a unique candidate to study binary orbital and accretion disk dynamics in high powered X-ray sources. We observed the X-ray source in 4U 1822−371 with the Chandra High Energy Transmission Grat...
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ژورنال
عنوان ژورنال: The Astrophysical Journal
سال: 2011
ISSN: 0004-637X,1538-4357
DOI: 10.1088/0004-637x/729/2/102