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LP 944-020 : ウィキペディア英語版
LP 944-20


LP 944-20 is a dim brown dwarf of spectral class M9 located about 21 light-years from the Solar System in the constellation of Fornax. With a visual apparent magnitude of 18,〔 it has one of the dimmest visual magnitudes listed on the RECONS page.
On 15 December 1999 a flare was detected.〔http://www.solstation.com/stars/lp944-20.jpg〕
==Distance==
The first parallax measurement from 1996 found that LP 944-20 (designated there as BRI 0337−3535) has a relative parallax of \pi_r=200.0\pm4.2 mas, and its correction from relative to absolute parallax (i.e. mean parallax of the reference frame stars) is \pi_=1.4\pm0.3 mas. This yields an absolute parallax of \pi_r+\pi_=200.0+1.4=201.4 mas, with a standard deviation (according to \sigma_^2=\sigma_X^2+\sigma_Y^2〔(Mean and Variance of Random Variables )〕) of \sqrt}^2}=\sqrt=4.21 mas, which corresponds to a distance of pc, or ly.〔
〕 (The same values of absolute parallax and its standard deviation are in the RECONS' TOP100 list.〔In RECONS' TOP100 older versions the standard deviation value was 4.20 mas, not 4.21 mas.〕
A newer parallax, published in 2013, is mas ( pc or ly).〔

抄文引用元・出典: フリー百科事典『 ウィキペディア(Wikipedia)
ウィキペディアで「LP 944-20」の詳細全文を読む



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