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20182026
most citedThe size, shape, density and ring of the dwarf planet Haumea from a stellar occultation

258 citations · 436 across the 18 of their papers we have counts for

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11 papers · 1 filter

astro-ph.SR2023★ 12 cited

BU Canis Minoris -- the Most Compact Known Flat Doubly Eclipsing Quadruple System

Theodor Pribulla, Tamás Borkovits, Rahul Jayaraman +25

We have found that the 2+2 quadruple star system BU CMi is currently the most compact quadruple system known, with an extremely short outer period of only 121 days. The previous re…

astro-ph.SR2023★ 23 cited

A Study of Nine Triply Eclipsing Triples

S. A. Rappaport, T. Borkovits, R. Gagliano +22

In this work we report the independent discovery and analysis of nine new compact triply eclipsing triple star systems found with the TESS mission: TICs 47151245, 81525800, 9901326…

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.SR2021★ 7 cited

V680 Mon -- a young mercury-manganese star in an eclipsing heartbeat system

E. Paunzen, S. Huemmerich, M. Fedurco +3

Chemically peculiar stars in eclipsing binary systems are rare objects that allow the derivation of fundamental stellar parameters and important information on the evolutionary sta…

astro-ph.SR2020★ 15 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.SR2020★ 1 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…