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 35
... nebula and nucleus were brighter than that star . At every observation since the nebulosity has been a striking object - the colour of nebula and nucleus being a bluish white - quite in contrast to the star F , which has appeared ...
... nebula and nucleus were brighter than that star . At every observation since the nebulosity has been a striking object - the colour of nebula and nucleus being a bluish white - quite in contrast to the star F , which has appeared ...
Page 39
... nebula , and shows that the dark markings which begin at the centre of the mass extend in curiously mean- dering lines to great distances , in several places enclosing nearly circular spaces . Looking at this photograph the nebula seems ...
... nebula , and shows that the dark markings which begin at the centre of the mass extend in curiously mean- dering lines to great distances , in several places enclosing nearly circular spaces . Looking at this photograph the nebula seems ...
Page 55
... nebula . By Eugen von Gothard . In the new star , which appeared in February , a catastrophe took place before our eyes , which is perhaps destined to afford us a glimpse into the origin and the disappearance of celestial bodies . My ...
... nebula . By Eugen von Gothard . In the new star , which appeared in February , a catastrophe took place before our eyes , which is perhaps destined to afford us a glimpse into the origin and the disappearance of celestial bodies . My ...
Page 56
... would be quite as impossible to take with the spectroscope most of the above - mentioned nebulæ , on account of the great feebleness of their lights . Great Nebula of Orion . 2 I. II . 486.1 56 LIII . 2 , Herr von Gothard , On the Spectrum.
... would be quite as impossible to take with the spectroscope most of the above - mentioned nebulæ , on account of the great feebleness of their lights . Great Nebula of Orion . 2 I. II . 486.1 56 LIII . 2 , Herr von Gothard , On the Spectrum.
Page 57
... nebular lines , λ = 5008 and 386 7μμ . are found in all the nebula which I have so far examined ; the third line , λ = 372'4 , occurs frequently , but another line , λ = 464–470μμ , appears but seldom . 4. The new star must , at present ...
... nebular lines , λ = 5008 and 386 7μμ . are found in all the nebula which I have so far examined ; the third line , λ = 372'4 , occurs frequently , but another line , λ = 464–470μμ , appears but seldom . 4. The new star must , at present ...
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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