Table 2: Orbit of BS Ind.
Period $1223\pm30$ days

Eccentricity $0.60\pm0.05$

$\omega$ $-6\pm2^\circ$

R₀ $10.8\pm0.2$ km s^-1

$f(m)={{M_2^3 \sin^3i}\over{(m_1+m_2)^2}}$ $0.273\pm0.06~M_\odot$

$a~\sin~i$ $2.7\pm0.2$ AU

m₁ $0.8\pm0.1~M_\odot$

m₂ $0.9\pm0.1~M_\odot$

periastron passage [JD] $2~450~489\pm30$

**Table 2:** Orbit of BS Ind.
Period	$1223\pm30$ days
Eccentricity	$0.60\pm0.05$
$\omega$	$-6\pm2^\circ$
R₀	$10.8\pm0.2$ km s^-1
$f(m)={{M_2^3 \sin^3i}\over{(m_1+m_2)^2}}$	$0.273\pm0.06~M_\odot$
$a~\sin~i$	$2.7\pm0.2$ AU
m₁	$0.8\pm0.1~M_\odot$
m₂	$0.9\pm0.1~M_\odot$
periastron passage [JD]	$2~450~489\pm30$

Source LaTeX | All tables | In the text

	1 Introduction
	2 The light-curve of BS Ind
	3 The long-period orbit
	4 The detection of the two eclipsing stars
	5 Conclusions
	References