Effect of Some Modified Models of Gravity on the Radial Velocity of Binary Systems

For many classes of astronomical and astrophysical binary systems, long observational records of their radial velocity <i>V</i>, which is their directly observable quantity, are available. For exoplanets close to their parent stars, they cover several full orbital revolutions, while for...

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Bibliographic Details
Main Authors: Lorenzo Iorio, Matteo Luca Ruggiero
Format: Article
Language:English
Published: MDPI AG 2022-08-01
Series:Universe
Subjects:
Online Access:https://www.mdpi.com/2218-1997/8/9/443