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One of the best possible ways to look for disk-Jet symbiosis in galacticBlack Holes is to study the correlation between X-ray and radio emissions.Beyond this study, is there any alternative way to trace the symbiosis? Toanswer, we investigated the X-ray features of few black hole candidates basedon the archival data of PCA/RXTE. We found evidences of `disappearance' of QPOsin the power density spectra and subsequent spectral softening of the energyspectra during the radio flares (i.e., `transient' Jets). We delve deep intothe nature of the accretion dynamics to understand the disk-Jet symbiosis.

Is the `disappearance' of low-frequency QPOs in the power spectra a general phenomenon for Disk-Jet symbiosis?