activity
20002005
most citedAE Aquarii: how CVs descend from supersoft binaries

120 citations · 393 across the 8 of their papers we have counts for

collaborators

9 papers

astro-ph2005★ 24 cited

The population of black widow pulsars

A. R. King, M. E. Beer, D. J. Rolfe +2

We consider the population of black widow pulsars (BWPs). The large majority of these are members of globular clusters. For minimum companion masses < 0.1 Msun, adiabatic evolution…

astro-ph2003★ 36 cited

A New Evolutionary Channel for Type Ia Supernovae

A. R. King, D. J. Rolfe, K. Schenker

We show that long-period dwarf novae offer a promising route for making Type Ia supernovae. For typical dwarf nova duty cycles d ~ 0.1 - 0.01, mass is accreted by the white dwarf m…

astro-ph2003

Thermal-timescale mass transfer and magnetic CVs

Klaus Schenker, Graham A. Wynn, Roland Speith

We investigate the spin evolution of the unusual magnetic CV AE Aqr. As a prototype for a potentially large population of CVs subject to a thermally unstable phase of mass transfer…

astro-ph2002★ 120 cited

AE Aquarii: how CVs descend from supersoft binaries

K. Schenker, A. R. King, U. Kolb +2

AE Aquarii is a propeller system. It has the shortest spin period among cataclysmic variables, and this is increasing on a 10^7 yr timescale. Its UV spectrum shows very strong carb…

astro-ph2002★ 87 cited

Blunting the Spike: the CV Minimum Period

A. R. King, K. Schenker, J. M. Hameury

The standard picture of CV secular evolution predicts a spike in the CV distribution near the observed short-period cutoff P_0 ~ 78 min, which is not observed. We show that an intr…

astro-ph2002★ 78 cited

The UV line spectrum of the soft X-ray transient XTE J1118+480: a CNO processed core exposed

C. A. Haswell, R. I. Hynes, A. R. King +1

We compare UV spectra of the recent soft X-ray transients XTE J1118+480 and XTE J1859+226. The emission line strengths in XTE J1118+480 strongly suggest that the accreting material…