On the orbit of γ centauri
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W. Doberck
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Article
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1905
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John Wiley and Sons
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English
⚖ 160 KB
The errors are large owing to the southern declination The following ephemeris has been calculated from of the star. elements II by aid of the formulae: Q C O S B = -0 ! 0 ~4 6 + 0 ! ' 5 1 4 6 s i n ( 1 ~~~~\* -E ) Q sin B = -0!'6661 + 1!2682 sin (79" 46' -E) f z = -o!'1947 + 1!'0297 sin (zoo 46' +