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www.aanda.org/articles/aa/abs/2025/02/aa51658-24/aa51658-24....PDF

Impact of accretor size on the morphology of supersonic, non-relativistic, axisymmetric Bondi-Hoyle-Lyttleton accretion flows

SA Jolehkaran, L Brendel, R Kuiper - Astronomy & Astrophysics, 2025 - aanda.org
۱ ارجاع2025

Context. Fast-moving accretors are a ubiquitous phenomenon in astrophysics. Their interaction with the surrounding gas can leave characteristic imprints on the form of morphological …

arxiv.org/abs/2502.08288PDF

Impact of accretor size on the morphology of supersonic Bondi-Hoyle-Lyttleton accretion flows

SA Jolehkaran, L Brendel, R Kuiper - arXiv preprint arXiv:2502.08288, 2025 - arxiv.org
۱ ارجاع2502

Fast-moving accretors are ubiquitous in astrophysics. Their interaction with surrounding gas leaves characteristic imprints, forming structures like bow shocks, Mach cones, and density …

journals.aps.org/prd/abstract/10.1103/PhysRevD.111.083010PDF

Effects of black hole environments on extreme mass-ratio hyperbolic encounters

YZ Cheng, Y Cao, Y Tang - Physical Review D, 2025 - APS
۹ ارجاع2025

Extreme mass-ratio hyperbolic encounters (EMRHEs) around the supermassive black holes will be observable at the future gravitational-wave (GW) detectors in space, such as LISA …

arxiv.org/abs/2606.31477PDF

Multi-wavelength Emission Modeling from Accretion Flows around Isolated Black Holes Including Magnetic Flux Transport

T Koshimizu, SS Kimura - arXiv preprint arXiv:2606.31477, 2026 - arxiv.org
2606

Isolated stellar-mass black holes (IBHs) are expected to be abundant in the Milky Way, yet their electromagnetic signatures remain largely undetected. We investigate the detectability of …

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