反驳高同心度行星HD 220773b

Ilaria Carleo, Silvano Desidera, Alessandro Sozzetti, Serena Benatti, Riccardo Claudi, Mario Damasso, Matteo Pinamonti and Alessandro Ruggeri
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摘要

据宣布,HD 220773 有一颗位于偏心轨道上的巨行星。行星系统全球结构合作组织利用伽利略国家望远镜的 HARPS-N 摄谱仪对这一目标进行了跟踪,以寻找该系统中的其他小行星。这一径向速度监测产生了大约 130 个 HARPS-N 数据点,从而驳斥了所宣布的行星。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Disproving the High-eccentricity Planet HD 220773b
HD 220773 has been announced to host a giant planet in an eccentric orbit. Global Architecture of Planetary Systems collaboration followed this target up with the HARPS-N spectrograph at Telescopio Nazionale Galileo, in order to search for additional small planets in the system. This radial velocity monitoring produced approximately 130 HARPS-N data points, leading to the refutation of the announced planet.
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