MG15 - Talk detail |
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Participant |
PAL, PARTHA SARATHI | |||||||
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Institution |
SCHOOL OF PHYSICS & ASTRONOMY, SUN YAT SEN UNIVERSITY - DA XUE LU, TANGJIA - ZHUHAI - GUANGDONG - China | |||||||
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Session |
AC1 |
Accepted |
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Order |
Time |
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Talk |
Poster abstract |
Title |
Accretion flow geometry from observational evidances of compact objects | |||||
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Abstract |
Low Mass X-ray Binaries are the end products of stellar evolution. Due to advancement of observational instruments LMXBs came up as enigmatic sources for their interesting variabilities. The variabilities are believed to be the reason for the variation in Two Component Accretion Flows. The accretion flow variation results the variation in geometry of the accretion disc. The variable observational evidences from LMXBs (e.g. GRS 1915+105, GRO J1650-44, GX 339-4 etc.) are analysed and explained as geometry of accretion flow variation near the compact object through a mass independent general picture. |
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