Monthly Notices of the Royal Astronomical Society, Volume 68; Volumes 1907-1908Priestley and Weale, 1908 Includes lists of additions to the Society's library, usually separately paged. |
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Page 5
... bright rays on the , H. G. Tomkins . 571 occultations of the Hyades by the , W. Heath 31 Uranus by the , in 1908 , A. M. W. Downing stars by the , in 1907 , observed at the Royal Ob . 127 servatory , Greenwich physical libration of the ...
... bright rays on the , H. G. Tomkins . 571 occultations of the Hyades by the , W. Heath 31 Uranus by the , in 1908 , A. M. W. Downing stars by the , in 1907 , observed at the Royal Ob . 127 servatory , Greenwich physical libration of the ...
Page 9
... bright rays Transit instrument , on an improved method of illuminating the field in , Sir W. H. M. and H. A. H. Christie Treasurer's account for 1907 Trépied , Charles , obituary notice of .. Trust funds 28 287 396 571 181 222 252 224 ...
... bright rays Transit instrument , on an improved method of illuminating the field in , Sir W. H. M. and H. A. H. Christie Treasurer's account for 1907 Trépied , Charles , obituary notice of .. Trust funds 28 287 396 571 181 222 252 224 ...
Page 3
... bright bands of cyanogen at 3883 first discovered by Sir W. Huggins . It has generally been held that this incandescent cyanogen and the other carbon compounds evidenced by cometary spectra are emitted from the comet's head , driven out ...
... bright bands of cyanogen at 3883 first discovered by Sir W. Huggins . It has generally been held that this incandescent cyanogen and the other carbon compounds evidenced by cometary spectra are emitted from the comet's head , driven out ...
Page 8
... bright sky an exposure of 30 seconds was ample . The photographs obtained with the instrument exhibit the spectrum with very open scale , and many of the close double lines even in the cyanogen baud are well seen . The linear dispersion ...
... bright sky an exposure of 30 seconds was ample . The photographs obtained with the instrument exhibit the spectrum with very open scale , and many of the close double lines even in the cyanogen baud are well seen . The linear dispersion ...
Page 14
... bright line . Not displaced with respect to the chromosphere absorption line K3 . 4 < 2 +38 : : Ca Not Narrow bright line . displaced with respect to the chromosphere absorption line H3 . 4015'532 4017'925 I I Ti 4019'450 O I Co ...
... bright line . Not displaced with respect to the chromosphere absorption line K3 . 4 < 2 +38 : : Ca Not Narrow bright line . displaced with respect to the chromosphere absorption line H3 . 4015'532 4017'925 I I Ti 4019'450 O I Co ...
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Common terms and phrases
angle appear Astrographic axis bright brighter Cape Catalogue centre coefficient colour column comet comparison stars computed corrections correlation curve cyanogen David Gill deduced determination distance Double Stars drift E. E. Barnard Earth eclipse epoch equation equatorial faint formula give given Greenwich groups heliometer instrument Julian Day Jupiter latitude lens Lick Observatory limb lines longitude magnitude Max Wolf mean measures meridian method Monthly Notices Moon nebula nucleus number of stars observations obtained orbit outer condensation paper parallax Paris perihelion perihelion passage period perturbations photographs planet plates position present Professor proper motion reduced reflector refraction refractor region right ascension ring Royal Observatory satellite Saturn seen Sept solar spectra spectral class spectroheliograph spectroscope spectrum spot stellar sun-spot Sun's surface Table telescope tion variable Yerkes Observatory zone ΙΟ