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K. E. Saavik Ford

3 papers here

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

author position
  • middle author2
  • last author1

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

fields
  • astro-ph.HE2
  • astro-ph.GA1
ORCID 0000-0002-5956-851X

identity via Semantic Scholar / OpenAlex

most citedIntermediate mass black holes in AGN disks II. Model predictions & observational constraints

183 citations · 210 across the 3 of their papers we have counts for

collaborators

3 papers

astro-ph.HE2016★ 5 cited

On the resonant detonation of sub-Chandrasekhar mass white dwarfs during binary inspiral

B. McKernan, K. E. S. Ford

White dwarfs (WDs) are believed to detonate via explosive Carbon-fusion in a Type Ia Supernova when their temperature and/or density reach the point where Carbon is ignited in a ru…

astro-ph.HE2014★ 22 cited

Stars as resonant absorbers of gravitational waves

B. McKernan, K. E. S. Ford, B. Kocsis +1

Quadrupole oscillation modes in stars can resonate with incident gravitational waves (GWs), and grow non-linear at the expense of GW energy. Stars near massive black hole binaries…

astro-ph.GA2014★ 183 cited

Intermediate mass black holes in AGN disks II. Model predictions & observational constraints

B. McKernan, K. E. S. Ford, B. Kocsis +2

If intermediate mass black holes (IMBHs) grow efficiently in gas disks around supermassive black holes, their host active galactic nucleus (AGN) disks should exhibit myriad observa…

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