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researcher

Philip D. Hall

3 papers here

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

author position
  • first author2
  • middle author1

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

fields
  • astro-ph.SR3
ORCID 0000-0002-9460-2939
same name
  • Philip D. Hall — 1 paper, h 4

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
20142017
most citedEvolution models of helium white dwarf--main sequence star merger remnants

40 citations · 95 across the 3 of their papers we have counts for

collaborators

3 papers

astro-ph.SR2017★ 40 cited

Evolution models of helium white dwarf--main sequence star merger remnants

Xianfei Zhang, Philip D. Hall, C. Simon Jeffery +1

It is predicted that orbital decay by gravitational-wave radiation and tidal interaction will cause some close-binary stars to merge within a Hubble time. The merger of a helium-co…

astro-ph.SR2016★ 34 cited

Hydrogen in hot subdwarfs formed by double helium white dwarf mergers

Philip D. Hall, C. Simon Jeffery

Isolated hot subdwarfs might be formed by the merging of two helium-core white dwarfs. Before merging, helium-core white dwarfs have hydrogen-rich envelopes and some of this hydrog…

astro-ph.SR2014★ 21 cited

Core radii and common-envelope evolution

Philip D. Hall, Christopher A. Tout

Many classes of objects and events are thought to form in binary star systems after a phase in which a core and companion spiral to smaller separation inside a common envelope (CE)…

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