X-ray spectral state evolution in IGR J17091-3624 and comparison of its heartbeat oscillation properties with those of GRS 1915+105
Mayukh Pahari (TIFR, India), J. S. Yadav (TIFR, India), Sudip, Bhattacharyya (TIFR, India)

TL;DR
This paper investigates the spectral and timing evolution of IGR J17091-3624 during its 2011 outburst, highlighting its transition from typical BHXB states to heartbeat oscillations similar to GRS 1915+105, and compares their properties.
Contribution
It provides the first detailed comparison of heartbeat oscillation properties between IGR J17091-3624 and GRS 1915+105, revealing similarities in their variability patterns.
Findings
IGR J17091-3624 transitions from BHXB-like states to heartbeat oscillations.
Heartbeat oscillations in IGR J17091-3624 resemble those in GRS 1915+105.
Timing and spectral properties of heartbeat oscillations are quantitatively compared.
Abstract
In this work, we study the X-ray timing and spectral evolution of the transient low mass X-ray binary IGR J17091-3624 during first 66 days of its 2011 outburst. We present results obtained from observations with two instruments, Rossi X-ray Timing Explorer (RXTE)/Proportional Counter Array (PCA) and SWIFT/X-ray telescope (XRT), between 09 February, 2011 and 15 April, 2011. Using quasi-periodic oscillation classifications, power density spectrum characteristics, time-lag behavior and energy spectral properties, we determine source states and their transitions at different times of the outburst. During the first part of the evolution, the source followed trends usually observed from transient black hole X-ray binaries (BHXBs). Interestingly, a gradual transition is observed in IGR J17091-3624 from the low-variability SIMS, commonly seen in BHXBs, to a high-variability state with regular,…
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