activity
20192025
most citedHD 99458: First time ever Ap-type star as a Scuti pulsator in a short period eclipsing binary?

23 citations · 69 across the 10 of their papers we have counts for

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Showing astro-ph.SRShow all

11 papers · 1 filter

astro-ph.SR2025

The twin red giant branch system BD+20 5391 A case study of low-mass double-core evolution

M. Kurpas, M. Dorsch, S. Geier +12

Understanding interactions of binary systems on the red giant branch is crucial to understanding the formation of compact stellar remnants such as helium-core white dwarfs (He-WDs)…

astro-ph.SR2023

Density asymmetry and wind velocities in the orbital plane of the symbiotic binary EG Andromedae

N. Shagatova, A. Skopal, E. Kundra +4

Context. Non-dusty late-type giants without a corona and large-scale pulsations represent objects that do not fulfil the conditions under which standard mass-loss mechanisms can be…

astro-ph.SR20224 cited

Variability of eclipse timing:the case of V471 Tauri

Emil Kundra, Ľubomír Hambálek, Siegfried Vanaverbeke +4

The post-common envelope binary V471 Tauri has been an object of interest for decades. V471 Tau shows various phenomena due to its evolutionary state and unique properties, e.g. it…

astro-ph.SR2022

HD 183986: a high-contrast SB2 system with a pulsating component

Martin Vaňko, Theodor Pribulla, Pavol Gajdoš +7

There is a small group of peculiar early-type stars on the main sequence that show different rotation velocities from different spectral lines. This inconsistency might be due to t…

astro-ph.SR202015 cited

Wind mass transfer in S-type symbiotic binaries III. Confirmation of a wind focusing in EG Andromedae from the nebular [OIII]λ5007 line

N. Shagatova, A. Skopal, S. Yu. Shugarov +3

Context. The structure of the wind from the cool giants in symbiotic binaries carries important information for understanding the wind mass transfer to their white dwarf companions…

astro-ph.SR20201 cited

Close eclipsing binary BD And: a triple system

T. Pribulla, L. Hambalek, E. Guenther +5

BD And is a fairly bright (V = 10.8), active and close (P = 0.9258 days) eclipsing binary. The cyclic variability of the apparent orbital period as well as third light in the light…