Comprehensive analysis of AstroSat data shows a sign change in QPO time lags at ~2 Hz for high-inclination sources, consistent with a transition from elongated jet-like to compact corona.
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2 Pith papers cite this work. Polarity classification is still indexing.
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astro-ph.HE 2years
2026 2verdicts
UNVERDICTED 2representative citing papers
A synthesis of multi-wavelength observations and models of variability, jets, and polarization in stellar-mass black hole accretion systems.
citing papers explorer
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Understanding corona and disk evolution in black hole X-ray binaries through a comprehensive study of their broadband variability and QPO characteristics
Comprehensive analysis of AstroSat data shows a sign change in QPO time lags at ~2 Hz for high-inclination sources, consistent with a transition from elongated jet-like to compact corona.
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Accreting stellar-mass black holes
A synthesis of multi-wavelength observations and models of variability, jets, and polarization in stellar-mass black hole accretion systems.