| GAJDOŠ, Pavol, Martin VAŇKO, Theodor PRIBULLA, Daniel DUPKALA, Ján ŠUBJAK, Marek SKARKA, Petr KABÁTH, Lubomír HAMBÁLEK a Štefan PARIMUCHA. Transit timing variations, radial velocities, and long-term dynamical stability of the system Kepler-410. Monthly Notices of the Royal Astronomical Society. Oxford: OXFORD UNIV PRESS, 2019, roč. 484, č. 3, s. 4352-4359. ISSN 0035-8711. Dostupné z: https://dx.doi.org/10.1093/mnras/stz305. |
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@article{1512916,
author = {Gajdoš, Pavol and Vaňko, Martin and Pribulla, Theodor and Dupkala, Daniel and Šubjak, Ján and Skarka, Marek and Kabáth, Petr and Hambálek, Lubomír and Parimucha, Štefan},
article_location = {Oxford},
article_number = {3},
doi = {http://dx.doi.org/10.1093/mnras/stz305},
keywords = {planetary systems; planets and satellites: dynamical evolution andstability; techniques: radial velocities; methods: numerical; stars: individual: Kepler-410},
language = {eng},
issn = {0035-8711},
journal = {Monthly Notices of the Royal Astronomical Society},
title = {Transit timing variations, radial velocities, and long-term dynamical stability of the system Kepler-410},
url = {https://arxiv.org/pdf/1901.08485.pdf},
volume = {484},
year = {2019}
}
TY - JOUR
ID - 1512916
AU - Gajdoš, Pavol - Vaňko, Martin - Pribulla, Theodor - Dupkala, Daniel - Šubjak, Ján - Skarka, Marek - Kabáth, Petr - Hambálek, Lubomír - Parimucha, Štefan
PY - 2019
TI - Transit timing variations, radial velocities, and long-term dynamical stability of the system Kepler-410
JF - Monthly Notices of the Royal Astronomical Society
VL - 484
IS - 3
SP - 4352-4359
EP - 4352-4359
PB - OXFORD UNIV PRESS
SN - 00358711
KW - planetary systems
KW - planets and satellites: dynamical evolution andstability
KW - techniques: radial velocities
KW - methods: numerical
KW - stars: individual: Kepler-410
UR - https://arxiv.org/pdf/1901.08485.pdf
L2 - https://arxiv.org/pdf/1901.08485.pdf
N2 - Transit timing variations of Kepler-410Ab were already reported in a few papers.Their semi-amplitude is about 14.5 minutes. In our previous paper, we found thatthe transit timing variations could be caused by the presence of a stellar companionin this system. Our main motivation for this paper was to investigate variation in aradial-velocity curve generated by this additional star in the system. We performedspectroscopic observation of Kepler-410 using three telescopes in Slovakia and CzechRepublic. Using the cross-correlation function, we measured the radial velocities of thestar Kepler-410A. We did not observe any periodic variation in a radial-velocity curve.Therefore, we rejected our previous hypothesis about additional stellar companionin the Kepler-410 system. We ran different numerical simulations to study mean-motion resonances with Kepler-410Ab. Observed transit timing variations could bealso explained by the presence of a small planet near to mean-motion resonance 2:3with Kepler-410Ab. This resonance is stable on a long-time scale. We also looked forstable regions in the Kepler-410 system where another planet could exist for a longtime.
ER -
GAJDOŠ, Pavol, Martin VAŇKO, Theodor PRIBULLA, Daniel DUPKALA, Ján ŠUBJAK, Marek SKARKA, Petr KABÁTH, Lubomír HAMBÁLEK a Štefan PARIMUCHA. Transit timing variations, radial velocities, and long-term dynamical stability of the system Kepler-410. \textit{Monthly Notices of the Royal Astronomical Society}. Oxford: OXFORD UNIV PRESS, 2019, roč.~484, č.~3, s.~4352-4359. ISSN~0035-8711. Dostupné z: https://dx.doi.org/10.1093/mnras/stz305.
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