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Stellar wobble caused by a nearby binary system: eccentric and inclined orbits - MaRDI portal

Stellar wobble caused by a nearby binary system: eccentric and inclined orbits

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Publication:4905559

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DOI10.1051/0004-6361/201014812zbMath1260.85020arXiv1012.2375OpenAlexW2096490322WikidataQ58436410 ScholiaQ58436410MaRDI QIDQ4905559

Alexandre C. M. Correia, M. H. M. Morais

Publication date: 19 February 2013

Published in: Astronomy & Astrophysics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1012.2375

zbMATH Keywords

celestial mechanics planetary systems binaries: general radial velocities

Mathematics Subject Classification ID

Celestial mechanics (70F15) Galactic and stellar dynamics (85A05) Equations of motion in general relativity and gravitational theory (83C10)

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