
Physics and Astronomy Faculty Publications and Presentations
Document Type
Article
Publication Date
4-9-2025
Abstract
We present a unique discovery of three new detected systems showing two different phenomena together. These are 2+2 quadruple stellar systems showing two eclipsing binaries as the inner pairs. And besides that, these systems were also found to exhibit the precession of the inner orbits causing the inclination changes manifesting themselves through the eclipse depth variations. We are not aware of any similar known system on the sky nowadays, hence our discovery is really unique. In particular these systems are: CzeV4315 = HD 228777 (periods 6.7391 and 0.91932 d, inclination change of pair B of about 1.4∘ yr−1); ASASSN-V J075203.23−323102.7 = GDS_J0752031−323102 (8.86916 d + 2.6817 d, inclination change of pair B of about 1.03∘ yr−1, now only ellipsoidal variations); ASASSN-V J105824.33−611347.6 = TIC 465899856 (2.3304 d + 13.0033 d, inclination change of pair B, now undetectable). These systems provide us unique insight into the quadruple-star dynamics, including the orbit–orbit interaction, Kozai–Lidov cycles, and testing the stellar formation theories of these higher order multiples.
Recommended Citation
Zasche, P., Z. Henzl, M. Mašek, J. Kára, H. Kučáková, J. Merc, and R. Uhlař. "Three new 2+ 2 quadruple systems with changing inclination." Monthly Notices of the Royal Astronomical Society 539, no. 2 (2025): 1015-1023. https://doi.org/10.1093/mnras/staf495
Creative Commons License
This work is licensed under a Creative Commons Attribution 4.0 International License.
Publication Title
Monthly Notices of the Royal Astronomical Society
DOI
10.1093/mnras/staf495
Comments
Post doc publication.
© 2025 The Author(s). Published by Oxford University Press on behalf of Royal Astronomical Society. This is an Open Access article distributed under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0/), which permits unrestricted reuse, distribution, and reproduction in any medium, provided the original work is properly cited