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 54
... that the Nova is now about three magnitudes fainter photographically than visually . Royal Observatory , Greenwich : 1892 December 8 . On the Spectrum of the New Star in Auriga , 54 LIII . 2 , Mr. Christie , Nova Auriga .
... that the Nova is now about three magnitudes fainter photographically than visually . Royal Observatory , Greenwich : 1892 December 8 . On the Spectrum of the New Star in Auriga , 54 LIII . 2 , Mr. Christie , Nova Auriga .
Page 55
... spectrum of the new star several times directly by the eye , and six times by means of photography . The spectrum consisted of many bright and several dark lines , the latter mostly corresponding with the former . My photographs show 40 ...
... spectrum of the new star several times directly by the eye , and six times by means of photography . The spectrum consisted of many bright and several dark lines , the latter mostly corresponding with the former . My photographs show 40 ...
Page 56
... spectrum , the whole lengths , from 1500 to A372 , being only 2'4 mm . The resemblance between the spectra becomes ... spectrum and of the comparison spectrum . But it would be quite as impossible to take with the spectroscope most of ...
... spectrum , the whole lengths , from 1500 to A372 , being only 2'4 mm . The resemblance between the spectra becomes ... spectrum and of the comparison spectrum . But it would be quite as impossible to take with the spectroscope most of ...
Page 57
... spectrum , which seems to form the nucleus of the nebula . The spectrum gives the impression that this nucleus is surrounded by an extensive gaseous atmosphere . I will not draw any further conclusions at present , but will continue my ...
... spectrum , which seems to form the nucleus of the nebula . The spectrum gives the impression that this nucleus is surrounded by an extensive gaseous atmosphere . I will not draw any further conclusions at present , but will continue my ...
Page 60
... spectrum . I have been able to examine this star once since its re- appearance . On the morning of September 6 it was observed by Professor George E. Hale and myself with the 12 - inch of the Kenwood Observatory . At this time it was a ...
... spectrum . I have been able to examine this star once since its re- appearance . On the morning of September 6 it was observed by Professor George E. Hale and myself with the 12 - inch of the Kenwood Observatory . At this time it was a ...
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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