activity
20072026
most citedUnique sextuple system: 65 Ursae Majoris

194 citations · 1.2k across the 91 of their papers we have counts for

collaborators

94 papers

astro-ph.SR2026

Are there really some eccentric eclipsing binaries having orbital periods below 1 d?

P. Zasche, M. Wolf

The stellar binary systems are classical tools for studying dynamics, and tidal circularization is one of the processes taking place in these. During the last few years, several do…

astro-ph.SR2026

TIC 366240660 - A Dynamically Active Triple With a Very Short Outer Period of 30.5 Days

S. A. Rappaport, T. Borkovits, G. Torres +17

Methods: We analyze TESS photometric data, radial velocity measurements, and eclipse timing variation curves for the triple star system, TIC 366240660, with a photodynamical code t…

astro-ph.SR2026

Not so typical doubly eclipsing systems

Petr Zasche

Classical doubly eclipsing systems are stars for which two distinct eclipsing periods that apparently come from one point source are detected. Through thorough analysis, the physic…

astro-ph.SR2026

Large fraction of blends from Rowan et al. (2023)

P Zasche

Following the work by Rowan et al., I found that a large fraction of systems presented as triple/quadruple stars are in fact only blends. After careful inspection of 225 candidate…

astro-ph.SR2026

Refined reduction and standardisation of 53 years of UBV photometry at Hvar

Hrvoje Božić, Petr Harmanec, Miroslav Brož +17

Emission-line stars classified as Be exhibit light and colour variability on various timescales, ranging from days to decades. Their evolution must be constrained by long-term obse…

astro-ph.SR2026

Six new doubly eclipsing quadruples in a 2+2 architecture

P. Zasche, H. Kucakova, J. Kara +5

The study presents a confirmation of six quadruples with two sets of eclipses that have the 2+2 architecture. These so-called doubly eclipsing systems still present a quite rare gr…