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...
Main Authors: | , |
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Format: | Article |
Language: | English |
Published: |
MDPI AG
2022-08-01
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Series: | Universe |
Subjects: | |
Online Access: | https://www.mdpi.com/2218-1997/8/9/443 |