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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Page 13
... diameter is a possible explanation of this phenomenon ; for errors after the Full are deduced from observations of the second limb only , and before from those of the first . Now , if the adopted semi - diameter is too large , too large ...
... diameter is a possible explanation of this phenomenon ; for errors after the Full are deduced from observations of the second limb only , and before from those of the first . Now , if the adopted semi - diameter is too large , too large ...
Page 20
... diameter of the focal length . I would use such a framework as this , but double the length , with the telescope in one half and the counterpoise weights in the other . The centre of motion I would place exactly under and midway between ...
... diameter of the focal length . I would use such a framework as this , but double the length , with the telescope in one half and the counterpoise weights in the other . The centre of motion I would place exactly under and midway between ...
Page 27
... + const . given in the Monthly Notices , vol . lii . p . 146 , the measures of diameter of the four comparison stars being used to determine the value of the constant for each plate . Their Nov. 1892 . 27 Mr. Christie , On Nova Auriga .
... + const . given in the Monthly Notices , vol . lii . p . 146 , the measures of diameter of the four comparison stars being used to determine the value of the constant for each plate . Their Nov. 1892 . 27 Mr. Christie , On Nova Auriga .
Page 32
... which may be expected in determinations of magnitude deduced from measures of diameter of star - disks . Royal Observatory , Greenwich : 1892 November 11 . a , k , h a , k , h 32 Mr. Christie , On Nova Auriga . LIII . I ,
... which may be expected in determinations of magnitude deduced from measures of diameter of star - disks . Royal Observatory , Greenwich : 1892 November 11 . a , k , h a , k , h 32 Mr. Christie , On Nova Auriga . LIII . I ,
Page 35
... diameter , ' with a 10th - magnitude stellar nucleus . The nebulosity was very dense and whitish , and with a low power might escape notice . A setting of the wires gave the diameter of the nebu- losity as 3 " . The star nucleus was ...
... diameter , ' with a 10th - magnitude stellar nucleus . The nebulosity was very dense and whitish , and with a low power might escape notice . A setting of the wires gave the diameter of the nebu- losity as 3 " . The star nucleus was ...
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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