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John M. Blondin

3 papers here

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

author position
  • first author2
  • last author1

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

fields
  • astro-ph2
  • astro-ph.SR1
ORCID 0000-0001-9691-6803

identity via Semantic Scholar / OpenAlex

most citedLinear growth of spiral SASI modes in core-collapse supernovae

76 citations · 136 across the 3 of their papers we have counts for

collaborators

3 papers

astro-ph.SR2009★ 43 cited

Revisiting the Flip-Flop Instability of Hoyle-Lyttleton Accretion

John M. Blondin, T. Chris Pope

We revisit the flip-flop instability of two-dimensional planar accretion using high-fidelity numerical simulations. By starting from an initially steady-state axisymmetric solution…

astro-ph2006★ 76 cited

Linear growth of spiral SASI modes in core-collapse supernovae

John M. Blondin, Samantha Shaw

Two-dimensional axisymmetric simulations have shown that the post-bounce accretion shock in core collapse supernovae is subject to the Spherical Accretion Shock Instability, or SAS…

astro-ph2006★ 17 cited

X-Ray Emission from Planetary Nebulae Calculated by 1D Spherical Numerical Simulations

Muhammad Akashi, Noam Soker, Ehud Behar +1

We calculate the X-ray emission from both constant and time evolving shocked fast winds blown by the central stars of planetary nebulae (PNs) and compare with observations. Using s…

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