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researcher

Y. Sugawara

32 papers hereh-index 184.7k citations161 works total

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

author position
  • first author2
  • middle author11
  • last author2

Across the 15 of 32 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE24
  • astro-ph.IM3
  • astro-ph2
  • astro-ph.SR2
  • astro-ph.GA1
same name
  • Y. Sugawara — 3 papers, h 35
  • Y. Sugawara — 1 paper
  • Y. Sugawara — 1 paper, h 1
  • Y. Sugawara — 1 paper, h 3
  • Y. Sugawara — 1 paper, h 3

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
20072024
most citedThe Quiescent Intracluster Medium in the Core of the Perseus Cluster

500 citations · 1.7k across the 32 of their papers we have counts for

collaborators
Showing 2014Show all

4 papers · 1 filter

astro-ph.IM2014★ 55 cited

The ASTRO-H X-ray Astronomy Satellite

Tadayuki Takahashi, Kazuhisa Mitsuda, Richard Kelley +250

The joint JAXA/NASA ASTRO-H mission is the sixth in a series of highly successful X-ray missions developed by the Institute of Space and Astronautical Science (ISAS), with a planne…

astro-ph.HE2014

ASTRO-H White Paper - Stars -- Accretion, Shocks, Charge Exchanges and Magnetic Phenomena

Y. Tsuboi, K. Ishibashi, M. Audard +8

X-ray emission from stars has origins as diverse as the stars themselves: accretion shocks, shocks generated in wind-wind collisions, or release of magnetic energy. Although the sc…

astro-ph.SR2014★ 72 cited

Very Massive Stars in the Local Universe

Jorick S. Vink

Recent studies suggest the existence of very massive stars (VMS) up to 300 solar masses in the local Universe. As this finding may represent a paradigm shift for the canonical stel…

astro-ph.HE2014

3D Hydrodynamic & Radiative Transfer Models of X-ray Emission from Colliding Wind Binaries

Christopher M. P. Russell, Atsuo T. Okazaki, Stanley P. Owocki +3

Colliding wind binaries (CWBs) are unique laboratories for X-ray astrophysics. The massive stars in these systems possess powerful stellar winds with speeds up to ∼3000 km s$^…

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