Secular changes in the orbits of the quadruple system VW LMi. Issue 1 (13th March 2020)

• Record Type: Journal Article
• Authors: Pribulla, T; Puha, E; Borkovits, T; Budaj, J; Garai, Z; Guenther, E; Hambálek, L; Komžík, R; Kundra, E; Szabó, Gy M; Vaňko, M
• Is Part Of: Monthly notices of the Royal Astronomical Society. Volume 494:Issue 1(2020)
• Page Start: 178
• Page End: 189
• Publication Date: 2020-03-13
• Subjects: stars: binaries: eclipsing -- stars: binaries: spectroscopic -- stars: individual: VW LMi; Astronomy -- Periodicals; Periodicals; 520.5
• DOI: 10.1093/mnras/staa699
• Languages: English
• ISSNs: 0035-8711

Abstract

ABSTRACT: VW LMi is the tightest known quadruple system with 2 + 2 hierarchy. It consists of a W UMa-type eclipsing binary ( P 12 = 0.477 55 d) and another detached non-eclipsing binary ( P 34 = 7.93 d) orbiting around a common centre of mass in about P 1234 = 355 d. We present new observations of the system extending the time baseline to study long-term perturbations in the system and to improve orbital elements. The multidataset modelling of the system (four radial-velocity curves for the components and the timing data) clearly showed an apsidal motion in the non-eclipsing binary at a rate of 4.6 deg yr −1, but no other perturbations. This is consistent with the nearly co-planarity of the outer, 355-d orbit, and the 7.93-d orbit of the non-eclipsing binary. Extensive N -body simulations enabled us to constrain the mutual inclination of the non-eclipsing binary and the outer orbits to j 34–1234 < 10 deg.