2013/08/21 by A. Nandi, Nandi, A., D. Radhika +4
Physics and Astronomy · #Astrophysical Phenomena and Observations #Astrophysics and Cosmic Phenomena #FOS: Physical sciences #High Energy Astrophysical Phenomena (astro-ph.HE) #Pulsars and Gravitational Waves Research #astro-ph.HE
paper · pdf · doi:10.48550/arxiv.1308.4567
7 pages (restricted for proceedings publication), 5 colour figures. Accepted for proceedings of ASI Conference series of BASI
openalex publication_date 2013/08/21 · arxiv created 2013/09/08 · arxiv updated 2013/09/10 · openalex created_date 2016/06/24 · openalex updated_date 2026/07/28
One of the best possible ways to look for disk-Jet symbiosis in galactic Black Holes is to study the correlation between X-ray and radio emissions. Beyond this study, is there any alternative way to trace the symbiosis? To answer, we investigated the X-ray features of few black hole candidates based on the archival data of PCA/RXTE. We found evidences of `disappearance' of QPOs in the power density spectra and subsequent spectral softening of the energy spectra during the radio flares (i.e., `transient' Jets). We delve deep into the nature of the accretion dynamics to understand the disk-Jet symbiosis.