Monthly Notices of the Royal Astronomical Society, Volume 53; Volumes 1892-1893Priestley and Weale, 1893 Includes lists of additions to the Society's library, usually separately paged. |
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... Stars , by J. G. Porter , presented by the Cincinnati Observatory ; Oxford ... comparison has an important bearing on the determination of refraction . It ... comparison of the N.P.D.s for different years with the mean . The investigation ...
... Stars , by J. G. Porter , presented by the Cincinnati Observatory ; Oxford ... comparison has an important bearing on the determination of refraction . It ... comparison of the N.P.D.s for different years with the mean . The investigation ...
Page 3
... star is a rough indication of the time of year at ... stars observed below the pole must be regarded as having an R.A. differing by twelve hours from their tabular R.A. , and Table I. must be corrected accordingly . The original comparison ...
... star is a rough indication of the time of year at ... stars observed below the pole must be regarded as having an R.A. differing by twelve hours from their tabular R.A. , and Table I. must be corrected accordingly . The original comparison ...
Page 4
... compared with the Theoretical Variation of Latitude computed from Chandler's ... comparison is professedly only rough ; but , as it is distinctly favourable ... stars would have involved much labour , and it was , therefore , determined ...
... compared with the Theoretical Variation of Latitude computed from Chandler's ... comparison is professedly only rough ; but , as it is distinctly favourable ... stars would have involved much labour , and it was , therefore , determined ...
Page 27
... stars observed , 20. Number of quantities determined , 5 . Putting v here for the residuals , [ wvv ] = 0 ° 0251 ... comparison with four Argelander stars of 8-9 magnitude by means of the formula m = 25 ( log t - 0.97 √ ) + const ...
... stars observed , 20. Number of quantities determined , 5 . Putting v here for the residuals , [ wvv ] = 0 ° 0251 ... comparison with four Argelander stars of 8-9 magnitude by means of the formula m = 25 ( log t - 0.97 √ ) + const ...
Page 29
... star B.D. + 30 ° .898 , at the centre of the plate , the Nova in the second set being about 60 ' from that centre ... comparison stars referred to the mean of the four , which is assumed from Argelander to be 8:45 , Tables III . and ...
... star B.D. + 30 ° .898 , at the centre of the plate , the Nova in the second set being about 60 ' from that centre ... comparison stars referred to the mean of the four , which is assumed from Argelander to be 8:45 , Tables III . and ...
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Common terms and phrases
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