New inclination changing eclipsing binaries in the Magellanic Clouds

0499976 - FZÚ 2019 RIV FR eng J - Článek v odborném periodiku
Juryšek, Jakub - Zasche, P. - Wolf, M. - Vraštil, J. - Vokrouhlický, D. - Skarka, M. - Liška, J. - Janík, J. - Zejda, M. - Kurfürst, P. - Paunzen, E.
New inclination changing eclipsing binaries in the Magellanic Clouds.
Astronomy & Astrophysics. Roč. 609, Jan (2018), s. 1-30, č. článku A46. ISSN 0004-6361. E-ISSN 1432-0746
Institucionální podpora: RVO:68378271
Klíčová slova: binaries: eclipsing * stars: early-type * stars: fundamental parameters * Magellanic Clouds
Obor OECD: Astronomy (including astrophysics,space science)
Impakt faktor: 6.209, rok: 2018

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.
Trvalý link: http://hdl.handle.net/11104/0292156