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Extrasolar planets and brown dwarfs around A--F type stars. VIII. A giant planet orbiting the young star HD113337

机译:a - F型恒星周围的太阳系外行星和褐矮星。八。一个   巨行星绕着年轻的恒星HD113337轨道运行

摘要

In the frame of the search for extrasolar planets and brown dwarfs aroundearly-type main-sequence stars, we present the detection of a giant planetaround the young F-type star HD113337. We estimated the age of the system to be150 +100/-50 Myr. Interestingly, an IR excess attributed to a cold debris diskwas previously detected on this star. The SOPHIE spectrograph on the 1.93mtelescope at Observatoire de Haute-Provence was used to obtain ~300 spectraover 6 years. We used our SAFIR tool, dedicated to the spectra analysis of Aand F stars, to derive the radial velocity variations. The data reveal a 324.0+1.7/-3.3 days period that we attribute to a giant planet with a minimum massof 2.83 +- 0.24 Mjup in an eccentric orbit with e=0.46 +- 0.04. A long-termquadratic drift, that we assign to be probably of stellar origin, issuperimposed to the Keplerian solution.
机译:在寻找早期型主序恒星周围的太阳系外行星和褐矮星的过程中,我们提出了围绕年轻的F型恒星HD113337的巨型行星的探测。我们估计系统的使用年限为150 + 100 / -50 Myr。有趣的是,先前在该恒星上检测到归因于冷碎片盘的IR过量。上普罗旺斯天文台的1.93毫米望远镜上的SOPHIE光谱仪用于在6年中获得约300幅光谱。我们使用专用于A和F星光谱分析的SAFIR工具来推导径向速度变化。数据揭示了一个324.0 + 1.7 / -3.3天的周期,这归因于一个在e = 0.46±0.04的偏心轨道上具有2.83±0.24 Mjup的最小质量的巨型行星。我们认为可能是恒星起源的长期二次漂移与开普勒解叠加。

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