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@article{1390810,
author = {Jurýšek, Jakub and Zasche, Petr and Wolf, Marek and Vraštil, Jan and Vokrouhlický, David and Skarka, Marek and Liška, Jiří and Janík, Jan and Zejda, Miloslav and Kurfürst, Petr and Paunzen, Ernst},
article_number = {A46},
doi = {http://dx.doi.org/10.1051/0004-6361/201730655},
keywords = {binaries: eclipsing / stars: early-type / stars: fundamental parameters / Magellanic Cloud},
language = {eng},
issn = {1432-0746},
journal = {Astronomy & Astrophysics},
title = {New inclination changing eclipsing binaries in the Magellanic Clouds},
url = {https://doi.org/10.1051/0004-6361/201730655},
volume = {609},
year = {2018}
}
TY - JOUR
ID - 1390810
AU - Jurýšek, Jakub - Zasche, Petr - Wolf, Marek - Vraštil, Jan - Vokrouhlický, David - Skarka, Marek - Liška, Jiří - Janík, Jan - Zejda, Miloslav - Kurfürst, Petr - Paunzen, Ernst
PY - 2018
TI - New inclination changing eclipsing binaries in the Magellanic Clouds
JF - Astronomy & Astrophysics
VL - 609
IS - A46
SP - "nestránkováno"
EP - "nestránkováno"
SN - 14320746
KW - binaries: eclipsing / stars: early-type / stars: fundamental parameters / Magellanic Cloud
UR - https://doi.org/10.1051/0004-6361/201730655
L2 - https://doi.org/10.1051/0004-6361/201730655
N2 - Context. Multiple stellar systems are unique laboratories for astrophysics. Analysis of their orbital dynamics, if well characterized from their observations, may reveal invaluable information about the physical properties of the participating stars. Unfortunately, there are only a few known and well described multiple systems, this is even more so for systems located outside the Milky Way galaxy. A particularly interesting situation occurs when the inner binary in a compact triple system is eclipsing. This is because the stellar interaction, typically resulting in precession of orbital planes, may be observable as a variation of depth of the eclipses on a long timescale. Aims. We aim to present a novel method to determine compact triples using publicly available photometric data from large surveys. Here we apply it to eclipsing binaries (EBs) in Magellanic Clouds from OGLE III database. Our tool consists of identifying the cases where the orbital plane of EB evolves in accord with expectations from the interaction with a third star. Methods. We analyzed light curves (LCs) of 26121 LMC and 6138 SMC EBs with the goal to identify those for which the orbital inclination varies in time. Archival LCs of the selected systems, when complemented by our own observations with Danish 1.54-m telescope, were thoroughly analyzed using the PHOEBE program. This provided physical parameters of components of each system. Time dependence of the EB’s inclination was described using the theory of orbital-plane precession. By observing the parameter-dependence of the precession rate, we were able to constrain the third companion mass and its orbital period around EB. Results. We identified 58 candidates of new compact triples in Magellanic Clouds. This is the largest published sample of such systems so far. Eight of them were analyzed thoroughly and physical parameters of inner binary were determined together with an estimation of basic characteristics of the third star. Prior to our work, only one such system was well characterized outside the Milky Way galaxy. Therefore, we increased this sample in a significant way. These data may provide important clues about stellar formation mechanisms for objects with different metalicity than found in our galactic neighborhood.
ER -
JURÝŠEK, Jakub, Petr ZASCHE, Marek WOLF, Jan VRAŠTIL, David VOKROUHLICKÝ, Marek SKARKA, Jiří LIŠKA, Jan JANÍK, Miloslav ZEJDA, Petr KURFÜRST a Ernst PAUNZEN. New inclination changing eclipsing binaries in the Magellanic Clouds. \textit{Astronomy \&{} Astrophysics}. 2018, roč.~609, A46, s.~''nestránkováno'', 30 s. ISSN~1432-0746. Dostupné z: https://dx.doi.org/10.1051/0004-6361/201730655.
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