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Thomas Henderson and a Centauri

机译:托马斯亨德森和一名中心

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The first observations containing evidence of a measurable stellar parallax were made by Thomas Henderson at the Cape of Good Hope in 1832/33 Although his response to Manuel Johnson's discovery in early 1833, that a Cen has a large proper motion, was to intensify observations for his remaining month at the Cape, Henderson apparently saw no urgency to reduce his observations Instead he laboured through more routine matters, producing a catalogue of declinations of southern stars, improvements of refraction tables, and work on the solar and lunar parallaxes It was Bessel's announcement of a determination of the parallax of 61 Cyg that finally stirred Henderson into action in late 1838.
机译:含有可衡量的恒星视差的证据的第一个观察结果是由托马斯·亨德森于1832/33年在1832/33年在1833年初对Manuel Johnson发现的发现,即CEN具有大量适当的动议,是加强观察他剩下的居住月份,亨德森显然没有迫切地减少他的观察,而是通过更多的日常事项努力,制作南方恒星的拒绝目录,折射桌的改进,以及在太阳能和农历视差上的工作是贝塞尔的公告测定61个Cyg的视差,最终将亨德森搅拌成1838年后的作用。

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