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Ryosuke Hirai

3 papers here

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

author position
  • sole author1
  • first author1
  • middle author1

Across the 3 of 3 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE2
  • astro-ph.SR1
ORCID 0000-0002-8032-8174

identity via Semantic Scholar / OpenAlex

activity
20142019
most citedHydrodynamical simulations and similarity relations for eruptive mass loss from massive stars

40 citations · 94 across the 3 of their papers we have counts for

collaborators

3 papers

astro-ph.SR2019★ 40 cited

Hydrodynamical simulations and similarity relations for eruptive mass loss from massive stars

Stanley P. Owocki, Ryo Hirai, Philipp Podsiadlowski +1

Motivated by the eruptive mass loss inferred from Luminous Blue Variable (LBV) stars, we present 1D hydrodynamical simulations of the response from sudden energy injection into the…

astro-ph.HE2017★ 17 cited

Formation Scenario of the Progenitor of iPTF13bvn Revisited

Ryosuke Hirai

The formation scenario of the progenitor of iPTF13bvn has been revisited. iPTF13bvn is unique in the sense that a corresponding pre-supernova image has been identified. This has en…

astro-ph.HE2014★ 37 cited

The Outcome of Supernovae in Massive Binaries; Removed Mass, and its Separation Dependence

Ryosuke Hirai, Hidetomo Sawai, Shoichi Yamada

The majority of massive stars are formed in binary systems. It is hence reasonable to expect that most core-collapse supernovae (CCSNe) take place in binaries and the existence of…

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