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The Planetary Companion of 61 Cygni

Book ID
109543544
Publisher
Nature Publishing Group
Year
1944
Tongue
English
Weight
134 KB
Volume
153
Category
Article
ISSN
0028-0836

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The spectra of the stars P Cygni and 3' Cassiopeiae can be explained in terms of electrical discharges in one or more localized cometary nebulae, similar to that photographed in Hubble's Variable Nebula associated with the star R Monocerotis, and in the planetary nebulae generally (Sd). 2 An explana

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I zo 0 . 0 0 2 5 1 1 7 . C O S 2 W --1.1112926 -0.0000027~c0s4a, Daher ist die Bahn der retrograden periodischen Bewegung : -I --1.2841254 ro + 0.0029023 .cos 2 w -0.000003 Icos 4 w Man hat weiter mit Benutzung dieses Integrals : W as, dw dt dw -0 ' -0.9497694 -O.OOOOOOO -0.6500533 I 5 -0.9495 384 -