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A. King

4 papers hereh-index 314 citations6 works total

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

author position
  • first author1
  • middle author1
  • last author2

Across the 4 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph3
  • astro-ph.GA1
same name
  • A. King — 136 papers, h 53
  • A. King — 53 papers, h 28
  • A. King — 42 papers, h 40
  • A. King — 24 papers, h 21
  • A. King — 21 papers, h 14
  • A. King — 15 papers, h 19

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
20002025
most citedUnveiling the Fast Acceleration of AGN-Driven Winds at Kiloparsec Scales

18 citations · 21 across the 4 of their papers we have counts for

collaborators

4 papers

astro-ph.GA2025★ 18 cited

Unveiling the Fast Acceleration of AGN-Driven Winds at Kiloparsec Scales

Cosimo Marconcini, Alessandro Marconi, Giovanni Cresci +18

Supermassive black holes at the centre of galaxies gain mass through accretion disks. Models predict that quasi-spherical winds, expelled by the black hole during active accretion…

astro-ph2001★ 1 cited

A New Evolutionary Picture for CVs and LMXBs II. The Impact of Thermal-Timescale Mass Transfer

Klaus Schenker, Andrew R. King

Depending on the outcome of pre-CV formation, mass transfer may set in under thermally unstable conditions in a significant number of systems. Full computations have shown that suc…

astro-ph2001

A New Evolutionary Picture for CVs and LMXBs

Andrew R. King, Klaus Schenker

We consider an alternative to the standard picture of CV and LMXB evolution, namely the idea that most CVs (and by extension LMXBs) may not yet have had time to evolve to their the…

astro-ph2000★ 2 cited

Assisted stellar suicide: the wind-driven evolution of the recurrent nova T Pyxidis

C. Knigge, A. R. King, J. Patterson

We show that the extremely high luminosity of the short-period recurrent nova T Pyx in quiescence can be understood if this system is a wind-driven supersoft x-ray source (SSS). In…

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