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20152020
most citedThree in one go: consequential angular momentum loss can solve major problems of CV evolution

128 citations · 270 across the 10 of their papers we have counts for

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Showing astro-ph.SRShow all

5 papers · 1 filter

astro-ph.SR2018★ 24 cited

The consequences of a nearby supernova on the early Solar System

Simon Portegies Zwart, Inti Pelupessy, Arjen van Elteren +2

If the Sun was born in a relatively compact open cluster, it is quite likely that a massive (10MSun) star was nearby when it exploded in a supernova. The repercussions of a superno…

astro-ph.SR2017★ 19 cited

Characterising face-on accretion onto and the subsequent contraction of protoplanetary discs

T. P. G. Wijnen, O. R. Pols, F. I. Pelupessy +1

Observations indicate that stars generally lose their protoplanetary discs on a timescale of about 5 Myr. Which mechanisms are responsible for the disc dissipation is still debated…

astro-ph.SR2015

Empirical consequential angular momentum loss can solve long standing problems of CV evolution

Matthias R. Schreiber, Monica Zorotovic, Thomas P. G. Wijnen

The observed orbital period distribution of cataclysmic variables (CVs), the space density derived from observations, and the observed orbital period minimum are known to disagree…

astro-ph.SR2015★ 128 cited

Three in one go: consequential angular momentum loss can solve major problems of CV evolution

Matthias R. Schreiber, Monica Zorotovic, Thomas P. G. Wijnen

The average white dwarf (WD) masses in cataclysmic variables (CVs) have been measured to significantly exceed those of single WDs, which is the opposite of what is theoretically ex…

astro-ph.SR2015★ 39 cited

White dwarf masses in cataclysmic variables

T. P. G. Wijnen, M. Zorotovic, M. R. Schreiber

The white dwarf (WD) mass distribution of cataclysmic variables (CVs) has recently been found to dramatically disagree with the predictions of the standard CV formation model. The…