Abstract Details
| Name: YASHPAL BHULLA Affiliation: PACIFIC UNIVERSITY UDAIPUR Conference ID: ASI2017_423 Title : ACCRETION POWER OF TRANSIENT BLACK HOLE Authors and Co-Authors : Research Guide: Prof.S N A JAAFFREY Affliation : Pacific University, Udaipur Abstract Type : Poster Abstract Category : Extragalactic astronomy Abstract : The Black Hole accretion power is due to stellar mass binary system accumulate the matter onto some objects under the influence of gravity. In this work, we discuss the two transient Black Hole sources GRS 1915 + 105 and 4U 1630 - 47 with the instrument of Rossi X-ray Timing Explorer. We detect a high amplitude variability including hard flares. The sources have tremendous luminosity is equal to or more than Eddington Limit. We also present a detailed of Q.P.O., Quality Factor, Timing Properties and evolution of GRS 1915 + 105 and 4U 1630 - 47. |