Non-Keplerian effects in precision radial velocity measurements of double-line spectroscopic binary stars: numerical simulations

P. Sybilski, M. Konacki, S. K. Kozłowski +1

Current precision in radial velocity (RV) measurements of binary stars reaches $\sim$2 ms${}^{-1}$. This level of precision means that RV models have to take into account additional…