Transit timing variations, radial velocities, and long-term
dynamical stability of the system Kepler-410

J 2019

Transit timing variations, radial velocities, and long-term dynamical stability of the system Kepler-410

GAJDOŠ, Pavol, Martin VAŇKO, Theodor PRIBULLA, Daniel DUPKALA, Ján ŠUBJAK et. al.

Základní údaje

Originální název

Transit timing variations, radial velocities, and long-term dynamical stability of the system Kepler-410

Autoři

GAJDOŠ, Pavol (garant), Martin VAŇKO, Theodor PRIBULLA, Daniel DUPKALA, Ján ŠUBJAK, Marek SKARKA (203 Česká republika, domácí), Petr KABÁTH (203 Česká republika), Lubomír HAMBÁLEK a Štefan PARIMUCHA

Vydání

Monthly Notices of the Royal Astronomical Society, Oxford, OXFORD UNIV PRESS, 2019, 0035-8711

Další údaje

Jazyk

angličtina

Typ výsledku

Článek v odborném periodiku

Obor

10308 Astronomy

Stát vydavatele

Česká republika

Utajení

není předmětem státního či obchodního tajemství

Odkazy

Full Text

Impakt faktor

Impact factor: 5.357

Kód RIV

RIV/00216224:14310/19:00109367

Organizační jednotka

Přírodovědecká fakulta

DOI

http://dx.doi.org/10.1093/mnras/stz305

UT WoS

000462410300109

Klíčová slova anglicky

planetary systems; planets and satellites: dynamical evolution andstability; techniques: radial velocities; methods: numerical; stars: individual: Kepler-410

Štítky

rivok

Příznaky

Mezinárodní význam, Recenzováno

Změněno: 23. 1. 2020 15:29, Mgr. Marie Šípková, DiS.

Anotace

V originále

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.

Návaznosti

EF16_027/0008360, projekt VaV

Název: Postdoc@MUNI

Citovat

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.

@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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