X-Ray Timing Properties of the Black Hole Candidate IGR J17091-3624 During the 2022 Outburst Onset with AstroSat

arXiv:2607.14337 · astro-ph.HE · Submitted 2026-07-15 · Read on arXiv

Sree Bhattacherjee, Biplob Sarkar

astro-ph.HE

Submitted: 2026-07-15

Comments: The manuscript is submitted to the proceedings of the International Conference on Innovative Research in Science, Engineering & Social Sciences 2026, School of Basic and Applied Sciences, The Assam Kaziranga University. Comments are welcome. 14 pages 6 figures

License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/

Terminology

• Large Area X-ray Proportional Counter — 3× in this paper
• Accretion Flows — 2× in this paper · explained in 1 episode
• Hardness-Intensity Diagram — 2× in this paper
• Accretion Disk Dynamics — 1× in this paper · explained in 1 episode
• Calibration — 1× in this paper · explained in 7 episodes
• Department of Science and Technology — 1× in this paper
• Trace — 1× in this paper · explained in 2 episodes

Related papers

• Accreting Neutron Stars in Low-Mass X-ray Binaries
• Numerical Studies of Accretion Flows onto a Neutron Star Engulfed in a Massive Star
• Early panchromatic spectra reveal helium in the thermonuclear supernova 2024kce
• Multiwavelength Classification of Chandra Sources in Omega Centauri
• Impact of the equation of state on core collapse supernovae I: the low- T/W instability
• Secular Evolution of Quasiperiodic Eruptions: eRO-QPE2