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首页> 外文期刊>Astronomy and astrophysics >The HARPS search for southern extra-solar planets - XXIV. Companions to HD?85390, HD?90156, and HD?103197: a Neptune analog and two intermediate-mass planets
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The HARPS search for southern extra-solar planets - XXIV. Companions to HD?85390, HD?90156, and HD?103197: a Neptune analog and two intermediate-mass planets

机译:HARPS搜寻南部太阳系外行星-XXIV。与HD?85390,HD?90156和HD?103197的同伴:一个海王星模拟物和两个中间质量行星

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摘要

We report the detection of three new extrasolar planets orbiting the solar type stars HD?85390, HD?90156 and HD?103197 with the HARPS spectrograph mounted on the ESO 3.6-m telescope at La?Silla observatory. HD?85390 has a planetary companion with a projected intermediate mass (42.0???M⊕) on a 788-day orbit (a?=?1.52?AU) with an eccentricity of 0.41, for which there is no analog in the solar system. A drift in the data indicates the presence of another companion on a long-period orbit, which is however not covered by our measurements. HD?90156 is orbited by a warm Neptune analog with a minimum mass of 17.98?M⊕ (1.05? ), a period of 49.8 days (a?=?0.25?AU), and an eccentricity of?0.31. HD?103197 has an intermediate-mass planet on a circular orbit (P?=?47.8 d, M sini?=?31.2???M⊕). We discuss the formation of planets of intermediate mass (~30–100?M⊕), which should be rare inside a few?AU according to core accretion formation models.
机译:我们报告说,使用安装在La?Silla天文台ESO 3.6米望远镜上的HARPS光谱仪,探测到绕太阳系恒星HD?85390,HD?90156和HD?103197的三个新太阳系外行星。 HD?85390有一个行星伴星,在788天的轨道(a?=?1.52?AU)上具有预计的中间质量(42.0 ??? M?),偏心率为0.41,在太阳系中没有类似物。系统。数据的漂移表明在长周期轨道上存在另一个伴星,但是我们的测量未涵盖它。 HD?90156由质量最低的17.98?M?(1.05?),49.8天(a?=?0.25?AU)和偏心距为0.31的海王星类似物绕轨道运行。 HD?103197在圆轨道上有一个中等质量的行星(P?=?47.8 d,M?sini?=?31.2?M?)。我们讨论了中等质量(〜30–100?M⊕)的行星的形成,根据核心吸积形成模型,这在少数几个AU内应该很少见。

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