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researcher

K. Shen

70 papers hereh-index 323.8k citations79 works total

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

author position
  • sole author1
  • first author17
  • middle author39
  • last author9

Across the 66 of 70 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE38
  • astro-ph.SR26
  • astro-ph.CO3
  • astro-ph2
  • astro-ph.GA1
same name
  • K. Shen — 41 papers, h 33
  • K. Shen — 41 papers, h 18
  • K. Shen — 35 papers, h 9
  • K. Shen — 12 papers, h 11
  • K. Shen — 11 papers, h 10
  • K. Shen — 7 papers, h 5

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 citedFaint Thermonuclear Supernovae from AM Canum Venaticorum Binaries

411 citations · 5.4k across the 69 of their papers we have counts for

collaborators
Showing 2009Show all

3 papers · 1 filter

astro-ph.HE2009★ 27 cited

Helium White Dwarfs in Cataclysmic Variables

Ken J. Shen, Irit Idan, Lars Bildsten

Binary evolution predicts a population of helium core (M < 0.5 Msol) white dwarfs (WDs) that are slowly accreting hydrogen-rich material from low mass main sequence or brown dwarf…

astro-ph.HE2009★ 349 cited

A faint type of supernova from a white dwarf with a helium-rich companion

H. B. Perets, A. Gal-Yam, P. Mazzali +25

Supernovae (SNe) are thought to arise from two different physical processes. The cores of massive, short-lived stars undergo gravitational core collapse and typically eject a few s…

astro-ph.HE2009★ 169 cited

Unstable Helium Shell Burning on Accreting White Dwarfs

Ken J. Shen, Lars Bildsten

AM Canum Venaticorum (AM CVn) binaries consist of a degenerate helium donor and a helium, C/O, or O/Ne WD accretor, with accretion rates of Mdot = 1e-13 - 1e-5 Msol/yr. For accreti…

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