E
Emese Forgács-Dajka
Researcher at Eötvös Loránd University
Publications - 5
Citations - 226
Emese Forgács-Dajka is an academic researcher from Eötvös Loránd University. The author has contributed to research in topics: Orbital elements & Perturbation (astronomy). The author has an hindex of 5, co-authored 5 publications receiving 202 citations. Previous affiliations of Emese Forgács-Dajka include University of Vienna.
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Journal ArticleDOI
Dynamical masses, absolute radii and 3D orbits of the triply eclipsing star HD 181068 from Kepler photometry
Tamás Borkovits,Tamás Borkovits,Aliz Derekas,Aliz Derekas,László L. Kiss,László L. Kiss,László L. Kiss,Amanda Király,Amanda Király,Emese Forgács-Dajka,Emese Forgács-Dajka,I. B. Biro,Timothy R. Bedding,Stephen T. Bryson,Daniel Huber,Daniel Huber,Róbert Szabó +16 more
TL;DR: In this article, a novel approach was proposed to determine absolute physical parameters (including masses and radii) and full orbital configuration of a triply eclipsing hierarchical triple star in the Kepler field, and the results indicated that the close and wide subsystems revolve in almost exactly coplanar and prograde orbits.
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Transit timing variations in eccentric hierarchical triple exoplanetary systems - I. Perturbations on the time scale of the orbital period of the perturber
TL;DR: In this paper, an analytical form of the O−C diagram, which describes transit timing variations (TTVs) in transiting exoplanetary systems that contain another more distant (a 2 ǫ −a 1 ) planetary or stellar companion, was given.
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Transit timing variations in eccentric hierarchical triple exoplanetary systems. I. Perturbations on the time-scale of the orbital period of the perturber
TL;DR: In this paper, an analytical form of the O-C diagram, which describes the TTV-s in trigonometric series, valid for arbitrary mutual inclinations, up to the sixth order in the inner eccentricity, is given.
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Tidal and rotational effects in the perturbations of hierarchical triple stellar systems. II. Eccentric systems : the case of AS Camelopardalis
TL;DR: In this article, the perturbations of a relatively close third star o n a tidally distorted eccentric eclipsing binary were studied. But the effect of a hypothetical third companion on both the real and observed apsidal motion period was not considered.
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On some long time dynamical features of the Trojan asteroids of Jupiter
TL;DR: In this article, the equation of motion of long periodic libration around the Lagrangian point in the restricted three-body problem is investigated and the range of validity of an approximate analytical solution in the tadpole region is determined by numerical integration.