Monthly Notices of the Royal Astronomical Society, Volume 68; Volumes 1907-1908Priestley and Weale, 1908 Includes lists of additions to the society's library, usually separately paged. |
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Page 4
... magnitude of η Argûs , 1908 128 372 613 Instruments of the Observatory , note on the single equation which com- prises the theory of the , Sir R. Ball 171 International Union for Solar Research , papers of the computing bureau , No. 1 ...
... magnitude of η Argûs , 1908 128 372 613 Instruments of the Observatory , note on the single equation which com- prises the theory of the , Sir R. Ball 171 International Union for Solar Research , papers of the computing bureau , No. 1 ...
Page 8
... . 544 , 677 S Serpentis , note on the period of , H. H. Turner . 560 η Argûs , magnitude of , 1908 , R. T. A. Inues 613 Y Cephei , note on , Rev. J. G. Hagen ....... 676 PAGE Stein , Rev. J. , corrections to Professor Turner's ( 8 ) Index .
... . 544 , 677 S Serpentis , note on the period of , H. H. Turner . 560 η Argûs , magnitude of , 1908 , R. T. A. Inues 613 Y Cephei , note on , Rev. J. G. Hagen ....... 676 PAGE Stein , Rev. J. , corrections to Professor Turner's ( 8 ) Index .
Page 82
... magnitude than are the étoiles de repère . This should provide a powerful method of searching for systematic errors in the photo- graphic places of the planet and the value of the Solar Parallax derived from them . § 2. The published ...
... magnitude than are the étoiles de repère . This should provide a powerful method of searching for systematic errors in the photo- graphic places of the planet and the value of the Solar Parallax derived from them . § 2. The published ...
Page 85
... Magnitude Equation in the San Fernando and Toulouse Series . It was shown in S.P.P. No. 5 , p . 78 , that the Toulouse results have a large and nearly linear magnitude The separated results for the Greenwich plates have since been com ...
... Magnitude Equation in the San Fernando and Toulouse Series . It was shown in S.P.P. No. 5 , p . 78 , that the Toulouse results have a large and nearly linear magnitude The separated results for the Greenwich plates have since been com ...
Page 86
... magnitude equation . No further light has been thrown on the cause of this error . Corrections were obtained by plotting the results for successive magnitude groups ( loc . cit . ) , and drawing the best possible smooth curves through ...
... magnitude equation . No further light has been thrown on the cause of this error . Corrections were obtained by plotting the results for successive magnitude groups ( loc . cit . ) , and drawing the best possible smooth curves through ...
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angle appear Astrographic axis bright brighter calculated Cape Catalogue centre coefficient colour column comet comparison stars computed corrections correlation curve cyanogen David Gill deduced determination distance Double Stars drift E. E. Barnard Earth eclipse epoch equation equatorial faint formula give given Greenwich groups heliometer instrument Julian Day Jupiter latitude lens Lick Observatory limb lines longitude magnitude Max Wolf mean measures meridian method Monthly Notices Moon nebula nucleus number of stars observations obtained orbit outer condensation paper parallax Paris perihelion perihelion passage period perturbations photographs planet plates position Professor proper motion reduced reflector refraction refractor region right ascension ring Royal Observatory satellite Saturn seen Sept solar spectra spectral class spectroheliograph spectroscope spectrum spot stellar sun-spot Sun's surface Table telescope tion variable Yerkes Observatory zone ΟΣ دو