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researcher

K. Moore

12 papers hereh-index 11698 citations17 works total

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

author position
  • first author4
  • middle author5
  • last author3

Across the 12 of 12 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR7
  • astro-ph.HE2
  • astro-ph.CO1
  • astro-ph.EP1
  • astro-ph.GA1
same name
  • K. Moore — 12 papers, h 47
  • K. Moore — 9 papers, h 8
  • K. Moore — 9 papers, h 7
  • K. Moore — 5 papers, h 28
  • K. Moore — 4 papers, h 24
  • K. Moore — 3 papers, h 20

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
20102018
most citedPTF11kx: A Type-Ia Supernova with a Symbiotic Nova Progenitor

351 citations · 946 across the 12 of their papers we have counts for

collaborators
Showing 2012Show all

3 papers · 1 filter

astro-ph.SR2012★ 43 cited

Circumstellar Shell Formation in Symbiotic Recurrent Novae

Kevin Moore, Lars Bildsten

We present models of spherically symmetric recurrent nova shells interacting with circumstellar material in a symbiotic system composed of a red giant expelling a wind, and a white…

astro-ph.CO2012★ 351 cited

PTF11kx: A Type-Ia Supernova with a Symbiotic Nova Progenitor

B. Dilday, D. A. Howell, S. B. Cenko +32

There is a consensus that Type-Ia supernovae (SNe Ia) arise from the thermonuclear explosion of white dwarf stars that accrete matter from a binary companion. However, direct obser…

astro-ph.SR2012★ 48 cited

Laterally Propagating Detonations in Thin Helium Layers on Accreting White Dwarfs

Dean M. Townsley, Kevin Moore, Lars Bildsten

Theoretical work has shown that intermediate mass (0.01Msun<M_He<0.1Msun) Helium shells will unstably ignite on the accreting white dwarf (WD) in an AM CVn binary. For more massive…

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