activity
20242026
collaborators

22 papers

astro-ph.HE2026

Production of High Energy Neutrinos in the Coronae of Ultraluminous X-ray Sources

Norita Kawanaka, Shigeo S. Kimura

We investigate the possibility of high-energy neutrino production in coronae associated with ultraluminous X-ray sources (ULXs) as super-Eddington accreting black holes. Adopting t…

astro-ph.HE2026

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

Takumi Koshimizu, Shigeo S. Kimura

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 detectabil…

astro-ph.HE2026

Discovery of CO Clouds Associated with the X-ray Jets of SS 433: Evidence for Shock-Cloud Interaction Enhancing Nonthermal X-ray Emission

Haruka Sakemi, Hidetoshi Sano, Yasuo Fukui +7

We report the first identification of molecular clumps directly associated with the re-brightening regions of the large-scale X-ray jets of SS 433, based on CO ( = 1--0)…

astro-ph.HE2026

Non-uniform particle injection into black hole jets by radiative magnetic reconnection

Rin Oikawa, Kenji Toma, Shigeo S. Kimura

Active galactic nuclei often exhibit highly collimated relativistic plasma outflows launched from the vicinity of their central black holes. One of the key theoretical challenges i…

astro-ph.HE2026

Little Red Dots as Hidden Neutrino Sources

Riku Kuze, Kunihito Ioka, Kohta Murase +2

Little Red Dots (LRDs) are enigmatic, compact, red galaxies at high redshift, -, discovered by the James Webb Space Telescope. Broad emission lines in the absence of X-…

astro-ph.HE2026

Super-knee cosmic rays from interacting supernovae

Nick Ekanger, Shigeo S. Kimura, Kazumi Kashiyama

There is increasing evidence that, in the very late phase of stellar evolution before core collapse, massive stars have winds with large mass loss rates that give rise to a dense c…