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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Results 1-5 of 36
Page 13
... centre " will be too small , and the error of the tables consequently a positive quantity ; while before the Full the reverse is the case . Again , the adopted semi - diameter may be large owing to the spurious border , due to ...
... centre " will be too small , and the error of the tables consequently a positive quantity ; while before the Full the reverse is the case . Again , the adopted semi - diameter may be large owing to the spurious border , due to ...
Page 20
... 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 20 LIII . I , Dr. Common , On the Best Form.
... 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 20 LIII . I , Dr. Common , On the Best Form.
Page 21
... centre of motion , causing a necessary movement of the observer of at the most 30 inches per hour . Instead of a tube connecting the mirrors it would only be necessary to have two lattice girders braced together at the top and bottom ...
... centre of motion , causing a necessary movement of the observer of at the most 30 inches per hour . Instead of a tube connecting the mirrors it would only be necessary to have two lattice girders braced together at the top and bottom ...
Page 22
... centre of motion of the telescope . Probable Error of the Clock Correction when both the Clock Rate and the Instrumental Constants are found by a Least Squares Solution of a Single Night's Observations . By the Rev. John T. Hedrick ...
... centre of motion of the telescope . Probable Error of the Clock Correction when both the Clock Rate and the Instrumental Constants are found by a Least Squares Solution of a Single Night's Observations . By the Rev. John T. Hedrick ...
Page 29
... centre of the plate , the Nova in the second set being about 60 ' from that centre . These plates were taken to test whether distance from the centre would appreciably affect the determination of photographic magnitude . The following ...
... centre of the plate , the Nova in the second set being about 60 ' from that centre . These plates were taken to test whether distance from the centre would appreciably affect the determination of photographic magnitude . The following ...
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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