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A Jupiter-mass planet around the K0 giant HD 208897

Authors :
I. F. Bikmaev
M. Yılmaz
E. N. Irtuganov
Varol Keskin
R. Ya. Zhuchkov
Selim O. Selam
Hideyuki Izumiura
I. Özavcı
A. I. Galeev
Eiji Kambe
S. Melnikov
Bun'ei Sato
Ege Üniversitesi
Publication Year :
2017
Publisher :
arXiv, 2017.

Abstract

WOS: 000416942200014<br />For over 10 years, we have carried out a precise radial velocity (RV) survey to find substellar companions around evolved G, K-type stars to extend our knowledge of planet formation and evolution. We performed high precision RV measurements for the giant star HD 208897 using an iodine (l(2)) absorption cell. The measurements were made at TUBlTAK National Observatory (TUG; RTT150) and Okayama Astrophysical Observatory (OAO). For the origin of the periodic variation seen in the RV data of the star, we adopted a Keplerian motion caused by an unseen companion. We found that the star hosts a planet with a minimum mass of m(2) sin i = 1.40 M-J, which is relatively low compared to those of known planets orbiting evolved intermediate-mass stars. The planet is in a nearly circular orbit with a period of P = 353 days at about 1 AU distance from the host star. The star is metal rich and located at the early phase of ascent along the red giant branch. The photometric observations of the star at Ankara University Kreiken Observatory (AUKR) and the HlPPARCOS photometry show no sign of variation with periods associated with the RV variation. Neither bisector velocity analysis nor analysis of the Ca II and H alpha lines shows any correlation with the RV measurements.<br />JSPS KAKENHIMinistry of Education, Culture, Sports, Science and Technology, Japan (MEXT)Japan Society for the Promotion of ScienceGrants-in-Aid for Scientific Research (KAKENHI) [JP23244038, JP16H02169]; Scientific and Technological Research Council of Turkey (TUBlTAK) [114F099]; [3.6714.2017/8.9]<br />This work was supported by The Scientific and Technological Research Council of Turkey (TUBlTAK), the project number of 114F099. Authors thank to TUG, KFU, and AST for partial support in using RTT150 (Russian-Turkish 1.5-m telescope in Antalya). This work was also supported by JSPS KAKENHI Grant Numbers JP23244038, JP16H02169. This work was funded by the subsidy 3.6714.2017/8.9 allocated to Kazan Federal University for the state assignment in the sphere of scientific activities.

Details

ISSN :
23244038
Database :
OpenAIRE
Accession number :
edsair.doi.dedup.....16a10c1c6eee1952c2ee085b7db7b518
Full Text :
https://doi.org/10.48550/arxiv.1708.01895