activity
19992022
most citedThe Uncertain Future of Massive Binaries Obscures the Origin of LIGO/Virgo Sources

71 citations · 160 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.SR2022★ 11 cited

Magnetically-gated accretion model: application to short bursts in the intermediate polar V1223 Sgr

J. -M. Hameury, J. -P. Lasota, A. W. Shaw

Some intermediate polars show outbursts that are much shorter than those observed in normal dwarf novae, and whose origin has remained unelucidated for a long time. We examine here…

astro-ph.HE2022★ 37 cited

Localised thermonuclear bursts from accreting magnetic white dwarfs

S. Scaringi, P. J. Groot, C. Knigge +16

Nova explosions are caused by global thermonuclear runaways triggered in the surface layers of accreting white dwarfs. It has been predicted that localised thermonuclear bursts on…

astro-ph.HE2021★ 71 cited

The Uncertain Future of Massive Binaries Obscures the Origin of LIGO/Virgo Sources

K. Belczynski, A. Romagnolo, A. Olejak +6

The LIGO/Virgo gravitational--wave observatories have detected 50 BH-BH coalescences. This sample is large enough to have allowed several recent studies to draw conclusions about t…

astro-ph.HE2015★ 41 cited

The slimming effect of advection on black-hole accretion flows

J. -P. Lasota, R. S. S. Vieira, A. Sadowski +2

At super-Eddington rates accretion flows onto black holes have been described as slim (aspect ratio ) or thick (H/R >1) discs, also known as tori or (Polish) doughn…

astro-ph1999

Maximum redshift and minimum rotation period of neutron stars

P. Haensel, J. P. Lasota, J. L. Zdunik

The lower bound on the period of uniform rotation of neutron stars (NS) with causal equation of state (EOS), P_ min, is shown to be determined, with a high precision, by the upper…

astro-ph1999

On the minimum period of uniformly rotating meutron stars

P. Haensel, J. P. Lasota, J. L. Zdunik

We show that the neutron star minimum period of rotation is determined, for causal equations of state, by the maximum value of the relativistic (compactness) parameter 2GM/Rc^2, al…