activity
20122022
most citedTesting the disk instability model of cataclysmic variables

76 citations · 243 across the 9 of their papers we have counts for

collaborators

9 papers

astro-ph.GA2022★ 24 cited

MOCCA: Dynamics and evolution of binary stars of multiple stellar populations in tidally filling and underfilling globular star clusters

Arkadiusz Hypki, Mirek Giersz, Jongsuk Hong +4

We present an upgraded version of the \MOCCA code for the study of dynamical evolution of globular clusters (GCs) and its first application to the study of evolution of multiple st…

astro-ph.SR2021★ 26 cited

The symbiotic recurrent nova V3890 Sgr: binary parameters and pre-outburst activity

J. Mikolajewska, K. Ilkiewicz, C. Galan +4

We present and analyze optical photometry and high resolution SALT spectra of the symbiotic recurrent nova V3890 Sgr at quiescence. The orbital period, P=747.6 days has been derive…

astro-ph.HE2018★ 76 cited

Testing the disk instability model of cataclysmic variables

Guillaume Dubus, Magdalena Otulakowska-Hypka, Jean-Pierre Lasota

The disk instability model attributes the outbursts of dwarf novae to a thermal-viscous instability of their accretion disk, an instability to which nova-like stars are not subject…

astro-ph.SR2018

SY Mus - search for physical parameters

Aleksandra Leśniewska, Magdalena Otulakowska-Hypka, Joanna Mikołajewska +1

This is a preliminary analysis of the orbital parameters of the well known eclipsing symbiotic binary, SY Muscae. It is a system composed of a white dwarf (WD) and a red giant (RG)…

astro-ph.SR2016★ 51 cited

Statistical analysis of properties of dwarf novae outbursts

Magdalena Otulakowska-Hypka, Arkadiusz Olech, Joseph Patterson

We present a statistical study of all measurable photometric features of a large sample of dwarf novae during their outbursts and superoutbursts. We used all accessible photometric…

astro-ph.SR2013★ 1 cited

Increasing supercycle lengths of active SU UMa-type dwarf novae

M. Otulakowska-Hypka, A. Olech

We present observational evidence that supercycle lengths of the most active SU UMa-type stars are increasing during the past decades. We analysed a large number of photometric mea…

astro-ph.SR2013★ 10 cited

On supercycle lengths of active SU UMa stars

M. Otulakowska-Hypka, A. Olech

We performed a detailed analysis of extensive photometric observations of a sample of most active dwarf novae, that is SU UMa stars which are characterised by supercycle lengths sh…

astro-ph.SR2012★ 13 cited

IX Draconis - a curious ER UMa-type dwarf nova

M. Otulakowska-Hypka, A. Olech, E. de Miguel +3

We report results of an extensive world-wide observing campaign devoted to a very active dwarf nova star - IX Draconis. We investigated photometric behaviour of the system to deriv…

astro-ph.SR2012★ 42 cited

The expanding dusty bipolar nebula around the nova V1280 Sco

Olivier Chesneau, E. Lagadec, M. Otulakowska-Hypka +15

V1280 Sco is one of the slowest dust-forming nova ever historically observed. We performed multi-epoch high-spatial resolution observations of the circumstellar dusty environment o…