On the stability of the detected planet in the triple system HD 131399

Barbara Funk; Elke Pilat-Lohinger; Akos Bazso; David Bancelin

On the stability of the detected planet in the triple system HD 131399

Barbara Funk, Elke Pilat-Lohinger, Akos Bazso, David Bancelin

Institut für Astrophysik

Veröffentlichungen: Beitrag in Buch › Beitrag in Konferenzband

Abstract

Wagner et al. (2016) reported the discovery of a Jovian planet within a triple-star system by using direct imaging. In their paper they suspect the planet might be on an unstable orbit. Due to the discovery by direct imaging the orbital parameters of the system (distances and eccentricities) possess large uncertainties. Therefore in our work we tested different dynamical configurations to determine the stable regions in the system HD 131399 by varying the distances and the eccentricities of the stellar and the planetary components. Using different numerical methods we could show that stable regions remain for almost all possible orbital parameters. Additionally we also investigated the possible habitability of the system HD 131399.

Originalsprache	Englisch
Titel	Proceedings of the First Greek-Austrian Workshop on Extrasolar Planetary Systems
Untertitel	held on the island of Ammouliani, Chalkidiki, Greece, September 18-25, 2016
Seiten	115 - 124
Seitenumfang	10
Publikationsstatus	Veröffentlicht - März 2017

ÖFOS 2012

103003 Astronomie
103004 Astrophysik

Andere Dateien und Links

http://adsabs.harvard.edu/abs/2017pfga.proc..115F

Zitationsweisen

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title = "On the stability of the detected planet in the triple system HD 131399",

abstract = "Wagner et al. (2016) reported the discovery of a Jovian planet within a triple-star system by using direct imaging. In their paper they suspect the planet might be on an unstable orbit. Due to the discovery by direct imaging the orbital parameters of the system (distances and eccentricities) possess large uncertainties. Therefore in our work we tested different dynamical configurations to determine the stable regions in the system HD 131399 by varying the distances and the eccentricities of the stellar and the planetary components. Using different numerical methods we could show that stable regions remain for almost all possible orbital parameters. Additionally we also investigated the possible habitability of the system HD 131399.",

author = "Barbara Funk and Elke Pilat-Lohinger and Akos Bazso and David Bancelin",

year = "2017",

month = mar,

language = "English",

isbn = "1544255632",

pages = "115 -- 124",

booktitle = "Proceedings of the First Greek-Austrian Workshop on Extrasolar Planetary Systems",

}

On the stability of the detected planet in the triple system HD 131399. / Funk, Barbara; Pilat-Lohinger, Elke; Bazso, Akos et al.
Proceedings of the First Greek-Austrian Workshop on Extrasolar Planetary Systems: held on the island of Ammouliani, Chalkidiki, Greece, September 18-25, 2016. 2017. S. 115 - 124.

Veröffentlichungen: Beitrag in Buch › Beitrag in Konferenzband

TY - GEN

T1 - On the stability of the detected planet in the triple system HD 131399

AU - Funk, Barbara

AU - Pilat-Lohinger, Elke

AU - Bazso, Akos

AU - Bancelin, David

PY - 2017/3

Y1 - 2017/3

N2 - Wagner et al. (2016) reported the discovery of a Jovian planet within a triple-star system by using direct imaging. In their paper they suspect the planet might be on an unstable orbit. Due to the discovery by direct imaging the orbital parameters of the system (distances and eccentricities) possess large uncertainties. Therefore in our work we tested different dynamical configurations to determine the stable regions in the system HD 131399 by varying the distances and the eccentricities of the stellar and the planetary components. Using different numerical methods we could show that stable regions remain for almost all possible orbital parameters. Additionally we also investigated the possible habitability of the system HD 131399.

AB - Wagner et al. (2016) reported the discovery of a Jovian planet within a triple-star system by using direct imaging. In their paper they suspect the planet might be on an unstable orbit. Due to the discovery by direct imaging the orbital parameters of the system (distances and eccentricities) possess large uncertainties. Therefore in our work we tested different dynamical configurations to determine the stable regions in the system HD 131399 by varying the distances and the eccentricities of the stellar and the planetary components. Using different numerical methods we could show that stable regions remain for almost all possible orbital parameters. Additionally we also investigated the possible habitability of the system HD 131399.

UR - http://adsabs.harvard.edu/abs/2017pfga.proc..115F

M3 - Contribution to proceedings

SN - 1544255632

SP - 115

EP - 124

BT - Proceedings of the First Greek-Austrian Workshop on Extrasolar Planetary Systems

ER -