Monthly Notices of the Royal Astronomical Society, Volume 53Priestley and Weale, 1893 Includes lists of additions to the society's library, usually separately paged. |
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Page 4
... determined to make some preliminary calculations before defi- nitely embarking on this enterprise . J. From the theoretical expressions given in Mr. Chandler's paper , above quoted , the epochs of maximum and minimum lati- tude were ...
... determined to make some preliminary calculations before defi- nitely embarking on this enterprise . J. From the theoretical expressions given in Mr. Chandler's paper , above quoted , the epochs of maximum and minimum lati- tude were ...
Page 17
... determined : - : - In which de = dv + dnz . And dv + 0 " 23-29 " · 35 T − 3 · 976 T2 . dnz = − ( V1 + V2 + M ) + ( 14 ′′ ́1 sin A + 0 ' ' ' 9 sin A ' ) 2 in which T is the number of centuries from the epoch of Hansen's Tables , viz ...
... determined : - : - In which de = dv + dnz . And dv + 0 " 23-29 " · 35 T − 3 · 976 T2 . dnz = − ( V1 + V2 + M ) + ( 14 ′′ ́1 sin A + 0 ' ' ' 9 sin A ' ) 2 in which T is the number of centuries from the epoch of Hansen's Tables , viz ...
Page 23
... determined as a linear function of the ns . Let AT = a'n ' + a''n ' ' + a ' " ' n ' " ' . α + p = B'n ' + B''n ' ' + B ' ' ' n ' ' ' + where a ' , B ' , & c . , are functions of the constant coefficients of the equations of condition ...
... determined as a linear function of the ns . Let AT = a'n ' + a''n ' ' + a ' " ' n ' " ' . α + p = B'n ' + B''n ' ' + B ' ' ' n ' ' ' + where a ' , B ' , & c . , are functions of the constant coefficients of the equations of condition ...
Page 26
... determined from the observations , ( 5 ) . If these quantities are found by a least squares solution , this epoch is before or after the epoch assumed for the constant clock correction by an interval which is the quotient of the co ...
... determined from the observations , ( 5 ) . If these quantities are found by a least squares solution , this epoch is before or after the epoch assumed for the constant clock correction by an interval which is the quotient of the co ...
Page 27
... determined , 5 . Putting here for the residuals , [ wvv ] = 0 * 0251 . For an observation of weight I , p2 = 0000761 = [ 6.8815 ] . Mean of the times of observation = 8h.98 . Assumed epoch of AT = 91.0 . [ ee . 4 ] 328 , ( PAT ) 2 = [ 6 ...
... determined , 5 . Putting here for the residuals , [ wvv ] = 0 * 0251 . For an observation of weight I , p2 = 0000761 = [ 6.8815 ] . Mean of the times of observation = 8h.98 . Assumed epoch of AT = 91.0 . [ ee . 4 ] 328 , ( PAT ) 2 = [ 6 ...
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Academy Andromedæ angle appeared Aquilæ Astronomer Royal Auriga Bisection bright Burnham Camelop Canis Carinæ Cassiopeia Catalogue Centauri centre Cephei cluster coefficient comet comparison stars correction Cygni Dembowski determined diameter distance double stars E. E. Barnard eclipse epoch Equat equatoreal exposure Galactic Long Geminorum Greenwich Greenwich Mean instrument Isaac Roberts June Jupiter Lalande lens Lick Observatory London longitude lunar Lupi Magn magnitude me²e mean measures Meteorological micrometer Monocerotis Monthly Notices Moon motion nebula Nova Auriga observations obtained Ophiuchi orbit Orionis paper parallax Paris period Persei photographs planet plates position probable error Professor proper motion Puppis Refraction right ascension Royal Observatory S. W. Burnham Sagittarii satellite Saturn Schiaparelli Scorpii seen Sept solar spectra spectroscope spectrum stellar Struve Tauri telescope thermometer tion transit transit circle Velorum ΙΟ