Die Hypothese des Energiegleichgewichtes in der Bahn für enge Doppelsternsysteme

DOI10.1002/ASNA.19552820304zbMath0065.45403OpenAlexW2017967226MaRDI QIDQ5850462

No author found.

Publication date: 1955

Published in: Astronomische Nachrichten (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1002/asna.19552820304

zbMATH Keywords

structure of matter

Cites Work

• On the Motion of the Apsidal Line in Close Binary Systems
• Apsidal Motion in Binary Stars
• The Non-radial Oscillations of Polytropic Stars

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