Orbite de l'étoile double β 962 = 26 Draconis

✍ Scribed by I. Balanovsky

• Publisher: John Wiley and Sons
• Year: 1908
• Tongue: English
• Weight: 148 KB
• Volume: 179
• Category: Article
• ISSN: 0004-6337
• DOI: 10.1002/asna.19081791905

✦ Synopsis

is about 90° it proves that the poles of the orbits lie near the pole of the great circle, and if the mean is 45" it indicates that the poles are accidentally distributed.

Calculating in this manner the mean of the nodes with reference to the ecliptic and galactic I obtain 41" in Orbite de l'e'toile double p 962 = 26 Draconis.

Par I. Balanovsky.

either case, which is near 45", but rather favours distribution along a great circle. We know only two poles without ambiguity (5 Cancri and 42 Comae). They both lie near the ecliptic. Depuis la dtcouverte de l'ttoile ,9962 (a = 1 7 ~3 3 ~4 4 ' d = +61O 58' [1880]) en 1879, elle a dtcrit un arc d'environ 1 5 0 ~. Pendant ce temps elle a t t t observte par divers astronomes. Nous en donnons ci-joint la liste des mesures, qui nous ont servi de base A determiner les Cltments de 1'o.rbite rtelle de cette ttoile double.

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