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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... Proper - motion Stars , by J. G. Porter , presented by the Cincinnati Observatory ; Oxford University Observatory , Researches in Stellar Parallax by the aid of Photo- graphy , Part 2 , presented by the Observatory ; H. Gyldén ...
... Proper - motion Stars , by J. G. Porter , presented by the Cincinnati Observatory ; Oxford University Observatory , Researches in Stellar Parallax by the aid of Photo- graphy , Part 2 , presented by the Observatory ; H. Gyldén ...
Page 22
... motion of the telescope . Probable Error of the Clock Correction when both the Clock Rate and the Instrumental ... proper method is to find the clock rate each night from that night's observations . Supposing that a least squares ...
... motion of the telescope . Probable Error of the Clock Correction when both the Clock Rate and the Instrumental ... proper method is to find the clock rate each night from that night's observations . Supposing that a least squares ...
Page 41
... proper motion of either star , or to the orbital movement of C about the close pair , can , of course , be wholly neglected , since that will be a constant quantity . In the interest of the solution of this question I have put these ...
... proper motion of either star , or to the orbital movement of C about the close pair , can , of course , be wholly neglected , since that will be a constant quantity . In the interest of the solution of this question I have put these ...
Page 64
... proper motion of the system . This is given by Stumpe from Argelander as o " 481 in the direction of 262 ° 95 . The place of this star ( 1880 ) is : Chicago : November 20 . R.A. 13h 43m 38 * Decl . 27 ° 35 ' The Lunar Eclipse , 1892 May ...
... proper motion of the system . This is given by Stumpe from Argelander as o " 481 in the direction of 262 ° 95 . The place of this star ( 1880 ) is : Chicago : November 20 . R.A. 13h 43m 38 * Decl . 27 ° 35 ' The Lunar Eclipse , 1892 May ...
Page 216
... suitable for employment as reference stars in connection with observations of minor planets and comets , but the places are sufficiently reliable for the determination of proper motions . In the introduction to this volume Professor ...
... suitable for employment as reference stars in connection with observations of minor planets and comets , but the places are sufficiently reliable for the determination of proper motions . In the introduction to this volume Professor ...
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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