Post-Keplerian effects on radial velocity in binary systems and the possibility of measuring General Relativity with the star S2 in 2018
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DOI: 10.1093/mnras/stx2134
Abstract: One of the directly measured quantities which are used in monitoring the orbital motions of many of the S stars revolving around the Supermassive Black Hole (SMBH) in the Galactic Center (GC) is their radial… read more here.
Keywords: radial velocity; star; textrm; post keplerian ... See more keywords