Search Results - "Kawanaka, Norita"
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Effects of Heat Conduction on Blocking off the Super-Eddington Growth of Black Holes at High Redshift
Published in The Astrophysical journal (01-09-2023)“…Abstract We investigate the effect of conductive heating of the gas surrounding a geometrically thick accretion disk on the growth of a black hole (BH) at high…”
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2
Radio emission from accreting isolated black holes in our galaxy
Published in Monthly notices of the Royal Astronomical Society (11-09-2019)“…ABSTRACT Apart from the few tens of stellar-mass black holes discovered in binary systems, an order of 108 isolated black holes (IBHs) are believed to be…”
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3
Cosmic-Ray Lithium Production at the Nova Eruptions Followed by a Type Ia Supernova
Published in Physical review letters (24-01-2018)“…Recent measurements of cosmic-ray (CR) light nuclei by AMS-02 have shown that there is an unexpected component of CR lithium whose spectral index is harder…”
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Search for a Black Hole Binary in Gaia DR3 Astrometric Binary Stars with Spectroscopic Data
Published in The Astrophysical journal (01-04-2023)“…Abstract We report the discovery of a candidate binary system consisting of a black hole (BH) and a red giant branch star in Gaia DR3. This binary system was…”
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Spatial and Binary Parameter Distributions of Black Hole Binaries in the Milky Way Detectable with Gaia
Published in The Astrophysical journal (01-08-2023)“…Abstract Soon after Gaia Data Release 3 (DR3) in 2022 June, some candidates (and one confirmed) of detached black hole (BH)–luminous companion (LC) binaries…”
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Detecting Black Hole Binaries by Gaia
Published in The Astrophysical journal (01-07-2018)“…We study the prospects of the Gaia satellite to identify black hole (BH) binary systems by detecting the orbital motion of the companion stars. Taking into…”
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Influence of Black Hole Kick Velocity on Microlensing Distributions
Published in The Astrophysical journal (01-09-2024)“…Abstract The natal kick velocity distribution for black holes (BHs) is unknown regardless of its importance for understanding the BH formation process…”
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X-ray detectability of accreting isolated black holes in our Galaxy
Published in Monthly notices of the Royal Astronomical Society (11-06-2018)“…Abstract Detectability of isolated black holes (IBHs) without a companion star but emitting X-rays by accretion from dense interstellar medium (ISM) or…”
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What determines the unique spectra of super-Eddington accretors? Origin of optically thick and low-temperature coronae in super-Eddington accretion flows
Published in Publications of the Astronomical Society of Japan (13-06-2021)“…Abstract The existence of relatively cool (kBT ≲ 10 keV) and optically thick (τ ≳ 3) coronae are inferred above super-Eddington accretion flow such as…”
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10
High-energy gamma-ray and neutrino production in star-forming galaxies across cosmic time: Difficulties in explaining the IceCube data
Published in Publications of the Astronomical Society of Japan (01-06-2018)“…Abstract We present new theoretical modeling to predict the luminosity and spectrum of gamma-ray and neutrino emission of a star-forming galaxy, from the star…”
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11
Magnetically Arrested Disks in Quiescent Black Hole Binaries: Formation Scenario, Observable Signatures, and Potential PeVatrons
Published in The Astrophysical journal (01-07-2021)“…Abstract We propose magnetically arrested disks (MADs) in quiescent (low-luminosity) black hole (BH) binaries as the origin of multiwavelength emission, and…”
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12
The Relationships between Active Galactic Nucleus Power and Molecular Gas Mass within 500 pc of the Center of Elliptical Galaxies
Published in The Astrophysical journal (01-03-2024)“…Abstract The physical quantity that directly controls the feedback of active galactic nuclei (AGNs) in elliptical galaxies remains to be determined. The…”
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JET LUMINOSITY FROM NEUTRINO-DOMINATED ACCRETION FLOWS IN GAMMA-RAY BURSTS
Published in The Astrophysical journal (20-03-2013)“…A hyperaccretion disk formed around a stellar-mass black hole is a plausible model for the central engine that powers gamma-ray bursts (GRBs). If the central…”
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14
Neutrino flavor ratios modified by cosmic-ray secondary acceleration
Published in Physical review. D, Particles, fields, gravitation, and cosmology (30-10-2015)Get full text
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15
A Relativistic Formula for the Multiple Scattering of Photons
Published in Astrophysical journal. Letters (01-05-2024)“…Abstract We have discovered analytical expressions for the probability density function (PDF) of photons that are multiply scattered in relativistic flows,…”
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16
TeV cosmic-ray electrons from millisecond pulsars
Published in Monthly notices of the Royal Astronomical Society (01-04-2012)“…Recent γ-ray observations by Fermi Gamma-Ray Space Telescope suggest that the γ-ray millisecond pulsar (MSP) population is separated into two subclasses with…”
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17
How does a secular instability grow in a hyperaccretion flow?
Published in Publications of the Astronomical Society of Japan (05-10-2015)“…Hyperaccretion flows with mass accretion rates far above the Eddington rate have an N-shaped equilibrium curve on the Σ– $\skew{3}\dot{M}$ plane (with Σ and…”
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18
Can the relativistic light-bending model explain X-ray spectral variations of Seyfert galaxies?
Published in Publications of the Astronomical Society of Japan (01-06-2018)“…Abstract Many Seyfert galaxies are known to exhibit Fe-K broad emission line features in their X-ray energy spectra. The observed lines have three distinct…”
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19
Positron annihilation as a cosmic ray probe
Published in Monthly notices of the Royal Astronomical Society. Letters (01-03-2012)“…ABSTRACT Recently, the gamma‐ray telescopes AGILE and Fermi observed several middle‐aged supernova remnants (SNRs) interacting with molecular clouds. A…”
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Dead Zone Formation and Nonsteady Hyperaccretion in Collapsar Disks: A Possible Origin of Short-Term Variability in the Prompt Emission of Gamma-Ray Bursts
Published in The Astrophysical journal (01-07-2007)“…The central engine of gamma-ray bursts (GRBs) is believed to be a hot and dense disk with hyperaccretion onto a few solar-mass black hole. We investigate where…”
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