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. |
From inside the book
Results 1-5 of 34
Page 12
... latter value , computed in May , which some- times differs slightly from the former , computed in February , is to be preferred ; for by May the observations of the previous year have been examined more thoroughly , and numerical errors ...
... latter value , computed in May , which some- times differs slightly from the former , computed in February , is to be preferred ; for by May the observations of the previous year have been examined more thoroughly , and numerical errors ...
Page 40
... latter especially brings the precipices , clefts , and valleys of the Apennines into striking prominence , on a scale which makes Archimedes 1 in . in diameter . Sydney Observatory : = 1892 September 17 . The Motion of Cancri . By S. W. ...
... latter especially brings the precipices , clefts , and valleys of the Apennines into striking prominence , on a scale which makes Archimedes 1 in . in diameter . Sydney Observatory : = 1892 September 17 . The Motion of Cancri . By S. W. ...
Page 55
... latter mostly corresponding with the former . My photographs show 40-43 bright lines and 12-13 dark ones . It appeared to me , therefore , as if it consisted of two bodies , of which the one produced the emission , the other the ...
... latter mostly corresponding with the former . My photographs show 40-43 bright lines and 12-13 dark ones . It appeared to me , therefore , as if it consisted of two bodies , of which the one produced the emission , the other the ...
Page 60
... latter part of August , it seems to have reached about 10 magnitude . This was followed by the important discovery by Professor E. E. Barnard , on the night of August 20 , that it was no longer a star , but was a small bright nebula ...
... latter part of August , it seems to have reached about 10 magnitude . This was followed by the important discovery by Professor E. E. Barnard , on the night of August 20 , that it was no longer a star , but was a small bright nebula ...
Page 65
... latter , as adopted in the Nautical Almanac , is undoubtedly too large - probably o " 6 too large at the distance with which we are here concerned - sɔ that the durations given below are probably too great in a corresponding proportion ...
... latter , as adopted in the Nautical Almanac , is undoubtedly too large - probably o " 6 too large at the distance with which we are here concerned - sɔ that the durations given below are probably too great in a corresponding proportion ...
Other editions - View all
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