THE PAN-PACIFIC PLANET SEARCH. VI. GIANT PLANETS ORBITING HD 86950 AND HD 222076
dc.contributor.author | Wittenmyer, Robert A. | |
dc.contributor.author | Jones, M. I. | |
dc.contributor.author | Zhao, Jinglin | |
dc.contributor.author | Marshall, J. P. | |
dc.contributor.author | Butler, R. P. | |
dc.contributor.author | Tinney, C. G. | |
dc.contributor.author | Wang, Liang | |
dc.contributor.author | Johnson, John Asher | |
dc.date.accessioned | 2024-01-10T14:22:04Z | |
dc.date.available | 2024-01-10T14:22:04Z | |
dc.date.issued | 2017 | |
dc.description.abstract | We report the detection of two new planets orbiting the K giants HD 86950 and HD 222076, based on precise radial velocities obtained with three instruments: AAT/UCLES, FEROS, and CHIRON. HD 86950b has a period of 1270 +/- 57 days at a=2.72 +/- 0.08 AU, and m sin i=3.6 +/- 0.7 M-Jup. HD 222076b has P=871 +/- 19 days at a=1.83 +/- 0.03 AU, and m sin i=1.56 +/- 0.11 M-Jup. These two giant planets are typical of the population of planets known to orbit evolved stars. In addition, we find a high-amplitude periodic velocity signal (K similar to 50 m/s(-1)) in HD 29399, and show that it is due to stellar variability rather than Keplerian reflex motion. We also investigate the relation between planet occurrence and host-star metallicity for the 164-star Pan-Pacific Planet Search sample of evolved stars. In spite of the small sample of PPPS detections, we confirm the trend of increasing planet occurrence as a function of metallicity found by other studies of planets orbiting evolved stars. | |
dc.description.funder | FONDECYT | |
dc.format.extent | 12 páginas | |
dc.fuente.origen | WOS | |
dc.identifier.doi | 10.3847/1538-3881/153/2/51 | |
dc.identifier.eissn | 1538-3881 | |
dc.identifier.issn | 0004-6256 | |
dc.identifier.uri | https://doi.org/10.3847/1538-3881/153/2/51 | |
dc.identifier.uri | https://repositorio.uc.cl/handle/11534/79851 | |
dc.identifier.wosid | WOS:000405781100001 | |
dc.information.autoruc | Física;Jones MI;S/I;1013827 | |
dc.issue.numero | 2 | |
dc.language.iso | en | |
dc.nota.acceso | Sin adjunto | |
dc.publisher | IOP PUBLISHING LTD | |
dc.revista | ASTRONOMICAL JOURNAL | |
dc.rights | registro bibliográfico | |
dc.subject | planetary systems | |
dc.subject | stars: individual(HD 29399, HD 86950, HD 222076) | |
dc.subject | techniques: radial velocities | |
dc.subject | PRECISE RADIAL-VELOCITIES | |
dc.subject | SPECTROSCOPIC STELLAR PARAMETERS | |
dc.subject | ALL-SKY SURVEY | |
dc.subject | EVOLVED STARS | |
dc.subject | HOST STAR | |
dc.subject | FUNDAMENTAL PARAMETERS | |
dc.subject | HABITABLE-ZONE | |
dc.subject | MASS STARS | |
dc.subject | METALLICITY | |
dc.subject | COMPANIONS | |
dc.subject.ods | 13 Climate Action | |
dc.subject.odspa | 13 Acción por el clima | |
dc.title | THE PAN-PACIFIC PLANET SEARCH. VI. GIANT PLANETS ORBITING HD 86950 AND HD 222076 | |
dc.type | artículo | |
dc.volumen | 153 | |
sipa.codpersvinculados | 1013827 | |
sipa.index | WOS | |
sipa.index | Scopus | |
sipa.trazabilidad | Carga SIPA;09-01-2024 |