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20122026
most citedRadiation Hydrodynamic Simulations of Line-Driven Disk Winds for Ultra Fast Outflows

74 citations · 539 across the 20 of their papers we have counts for

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10 papers · 1 filter

astro-ph.GA2024

Multiphase Gas Nature in the Sub-parsec Region of the Active Galactic Nuclei. III. Eddington Ratio Dependence on the Structures of Dusty and Dust-free Outflows

Yuki Kudoh, Keiichi Wada, Nozomu Kawakatu +1

We investigated the influence of the Eddington ratio on sub-parsec-scale outflows in active galactic nuclei (AGNs) with supermassive black holes (SMBHs) masses of M$_{\odot}…

astro-ph.GA2023★ 19 cited

Multiphase Gas Nature in the Sub-parsec Region of the Active Galactic Nuclei I: Dynamical Structures of Dusty and Dust-free Outflow

Yuki Kudoh, Keiichi Wada, Nozomu Kawakatu +1

We investigated dusty and dust-free gas dynamics for a radiation-driven sub-pc scale outflow in an active galactic nucleus (AGN) associated with a supermassive black hole $10^7 M_\…

astro-ph.GA2021★ 8 cited

Radiation hydrodynamics simulations of line-driven AGN disc winds: metallicity dependence and black hole growth

Mariko Nomura, Kazuyuki Omukai, Ken Ohsuga

Growth of the black holes (BHs) from the seeds to supermassive BHs (SMBHs, ) is not understood, but the mass accretion must have played an important role. We p…

astro-ph.GA2020★ 30 cited

The Fifth Candidate for an Intermediate-mass Black Hole in the Galactic Center

Shunya Takekawa, Tomoharu Oka, Yuhei Iwata +2

We report the results of high-resolution molecular line observations of the high-velocity compact cloud HCN-0.085-0.094 with the Atacama Large Millimeter/submillimeter Array. The H…

astro-ph.GA2019★ 12 cited

An energetic high-velocity compact cloud: CO0.31+0.11

Shunya Takekawa, Tomoharu Oka, Sekito Tokuyama +5

We have discovered an energetic high-velocity compact cloud CO0.31+0.11 in the central molecular zone of our Galaxy. CO0.31+0.11 is located at a projected distance of $\sim 4…

astro-ph.GA2018★ 45 cited

Indication of Another Intermediate-mass Black Hole in the Galactic Center

Shunya Takekawa, Tomoharu Oka, Yuhei Iwata +2

We report the discovery of molecular gas streams orbiting around an invisible massive object in the central region of our Galaxy, based on the high-resolution molecular line observ…

astro-ph.GA2018★ 9 cited

Magnetohydrodynamic Simulations of a Plunging Black Hole into a Molecular Cloud

Mariko Nomura, Tomoharu Oka, Masaya Yamada +4

Using two-dimensional magnetohydrodynamic simulations, we investigated the gas dynamics around a black hole plunging into a molecular cloud. In these calculations, we assumed a par…

astro-ph.GA2017★ 51 cited

Millimetre-wave Emission from an Intermediate-Mass Black Hole Candidate in the Milky Way

Tomoharu Oka, Shiho Tsujimoto, Yuhei Iwata +2

It is widely accepted that black holes (BHs) with masses greater than a million solar masses (Msun) lurk at the centres of massive galaxies. The origins of such `supermassive' blac…

astro-ph.GA2017★ 18 cited

Discovery of Two Small High-Velocity Compact Clouds in the Central 10 Parsecs of Our Galaxy

Shunya Takekawa, Tomoharu Oka, Yuhei Iwata +2

We discovered two small high-velocity compact clouds (HVCCs) in HCN and maps of the central 20 pc of our Galaxy. Both HVCCs have broad velocity widths ($ΔV \gtrsim…

astro-ph.GA2016★ 14 cited

Kinematics of Ultra-High-Velocity Gas in the Expanding Molecular Shell adjacent to the W44 Supernova Remnant

Masaya Yamada, Tomoharu Oka, Shunya Takekawa +6

We mapped the ultra-high-velocity feature (the "Bullet") detected in the expanding molecular shell associated with the W44 supernova remnant using the Nobeyama Radio Observatory 45…