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Table 3:

Basic physical properties of BU Tau as a single-line binary based on elliptical-orbit solution for the H$\alpha $ emission RVs - (cf. Table 2).

i
M2/M1 M2 A $A_{\rm peri.}$
($^\circ$)   ($M_{\odot}$) ($R_{\odot}$) ($R_{\odot}$)

90
0.0876 0.254 223.5 53.0
70 0.0936 0.272 223.9 53.1
50 0.1164 0.338 225.5 53.4

Notes. The estimates are derived assuming the primary mass of M1=2.9 $M_{\odot}$, A and $A_{\rm peri.}$ denote the semi-major axis and the binary separation at periastron, respectively.


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