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researcher

K. Asada

98 papers hereh-index 4312.8k citations163 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • first author5
  • middle author58
  • last author8

Across the 71 of 98 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE54
  • astro-ph.GA16
  • astro-ph.IM16
  • astro-ph6
  • astro-ph.CO4
  • gr-qc2
same name
  • K. Asada — 31 papers, h 11
  • K. Asada — 4 papers, h 5
  • K. Asada — 1 paper, h 3
  • K. Asada — 1 paper, h 4

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

activity
20022026
most citedFirst Sagittarius A* Event Horizon Telescope Results. I. The Shadow of the Supermassive Black Hole in the Center of the Milky Way

1.9k citations · 16.6k across the 97 of their papers we have counts for

collaborators
Showing 2017 · astro-ph.HEShow all

3 papers · 2 filters

astro-ph.HE2017★ 37 cited

Enhanced Polarized Emission from the One-Parsec-Scale Hotspot of 3C 84 as a Result of the Interaction with Clumpy Ambient Medium

H. Nagai, Y. Fujita, M. Nakamura +4

We present Very Long Baseline Array polarimetric observations of the innermost jet of 3C∼84 (NGC∼1275) at 43∼GHz. A significant polarized emission is detected at the…

astro-ph.HE2017★ 20 cited

Observable Emission Features of Black Hole GRMHD Jets on Event Horizon Scales

Hung-Yi Pu, Kinwah Wu, Ziri Younsi +3

The general-relativistic magnetohydrodynamical (GRMHD) formulation for black hole-powered jets naturally gives rise to a stagnation surface, wherefrom inflows and outflows along ma…

astro-ph.HE2017★ 19 cited

Lepton acceleration in the vicinity of the event horizon: Very-high-energy emissions from super-massive black holes

Kouichi Hirotani, Hung-Yi Pu, Lupin Chun-Che Lin +5

Around a rapidly rotating black hole (BH), when the plasma accretion rate is much less than the Eddington rate, the radiatively inefficient accretion flow (RIAF) cannot supply enou…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.