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19962022
most citedDwarf nova outbursts in intermediate polars

52 citations · 164 across the 8 of their papers we have counts for

collaborators

8 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.SR2021★ 17 cited

Modelling rebrightenings, reflares, and echoes in dwarf nova outbursts

J. -M. Hameury, J. -P. Lasota

The disc instability model accounts well for most of the observed properties of dwarf novae and soft X-ray transients, but the rebrightenings, reflares, and echoes occurring at the…

astro-ph.SR2020★ 16 cited

Modelling hystereses observed during dwarf-nova outbursts

J. -M. Hameury, C. Knigge, J. -P. Lasota +2

Context. Although the disc instability model is widely accepted as the explanation for dwarf nova outbursts, it is still necessary to confront its predictions to observations becau…

astro-ph.HE2018★ 19 cited

Disc instabilities and nova eruptions in symbiotic systems: RS Ophiuchi and Z Andromedae

D. A. Bollimpalli, J. -M. Hameury, J. -P. Lasota

Using the disc instability model for dwarf novae and soft X-ray transients, we investigate the stability of accretion discs in long-period binary systems. We simulate outbursts due…

astro-ph.SR2017★ 52 cited

Dwarf nova outbursts in intermediate polars

J. -M. Hameury, J. -P. Lasota

The disc instability model (DIM) has been very successful in explaining the dwarf nova outbursts observed in cataclysmic variables. When, as in intermediate polars (IP), the accret…

astro-ph.HE2017★ 17 cited

Hystereses in dwarf nova outbursts and low-mass X-ray binaries

J. -M. Hameury, J. -P. Lasota, C. Knigge +1

Context. The disc instability model (DIM) successfully explains why many accreting compact binary systems exhibit outbursts, during which their luminosity increases by orders of ma…

astro-ph.HE2016★ 15 cited

Outbursts in ultracompact X-ray binaries

J. -M. Hameury, J. -P. Lasota

Very faint X-ray binaries appear to be transient in many cases with peak luminosities much fainter than that of usual soft X-ray transients, but their nature still remains elusive.…

astro-ph1996★ 17 cited

Illumination in binaries

J. -M. Hameury, H. Ritter

We give a simple, but accurate method that can be used to account for illumination in compact binary systems which have a low-mass companion, even if spherically symmetric illumina…