Table 3: Multiple TTSs with SBs having a known orbit. The periodsof spectroscopic binary $P_{{\rm in}}$ (in days) and the angular distances (orperiods) of outer components are listed.
Source $P_{{\rm in}}$ $d_{{\rm out}}$ Remark

HD 155555 1.7 33 $^{\prime\prime}$

V1154 Sco 2.4 0 $.\!\!^{\prime\prime}$ 288

RW Aur 2.77 0 $.\!\!^{\prime\prime}$ 12 + 1 $.\!\!^{\prime\prime}$ 39 Quad.

RX J0529.4+0041 3.03 1 $.\!\!^{\prime\prime}$ 3 eclips.

RX J0541.4-0324 4.98 SB3

RX J1301.1-7654 13 1 $.\!\!^{\prime\prime}$ 44

UZ Tau 19.1 0 $.\!\!^{\prime\prime}$ 368 + 3 $.\!\!^{\prime\prime}$ 54 Quad.

HD 34700 23.5 5 $^{\prime\prime}$ + 10 $^{\prime\prime}$ Quad.

ROXs 42C 36 0 $.\!\!^{\prime\prime}$ 157

RX J0532.1-0732 46.9 SB3

V773 51.1 0 $.\!\!^{\prime\prime}$ 2 + 0 $.\!\!^{\prime\prime}$ 2 Trap.

Crux-3 58.3 4.6 yrs SB3

ROXs 43A 89.1 6 $^{\prime\prime}$

HD 98800 262 + 315 0 $.\!\!^{\prime\prime}$ 8 Quad.

Haro 1-14 591 12 $.\!\!^{\prime\prime}$ 9

**Table 3:** Multiple TTSs with SBs having a known orbit. The periodsof spectroscopic binary $P_{{\rm in}}$ (in days) and the angular distances (orperiods) of outer components are listed.
Source	$P_{{\rm in}}$	$d_{{\rm out}}$	Remark
HD 155555	1.7	33 $^{\prime\prime}$
V1154 Sco	2.4	0 $.\!\!^{\prime\prime}$ 288
RW Aur	2.77	0 $.\!\!^{\prime\prime}$ 12 + 1 $.\!\!^{\prime\prime}$ 39	Quad.
RX J0529.4+0041	3.03	1 $.\!\!^{\prime\prime}$ 3	eclips.
RX J0541.4-0324	4.98		SB3
RX J1301.1-7654	13	1 $.\!\!^{\prime\prime}$ 44
UZ Tau	19.1	0 $.\!\!^{\prime\prime}$ 368 + 3 $.\!\!^{\prime\prime}$ 54	Quad.
HD 34700	23.5	5 $^{\prime\prime}$ + 10 $^{\prime\prime}$	Quad.
ROXs 42C	36	0 $.\!\!^{\prime\prime}$ 157
RX J0532.1-0732	46.9		SB3
V773	51.1	0 $.\!\!^{\prime\prime}$ 2 + 0 $.\!\!^{\prime\prime}$ 2	Trap.
Crux-3	58.3	4.6 yrs	SB3
ROXs 43A	89.1	6 $^{\prime\prime}$
HD 98800	262 + 315	0 $.\!\!^{\prime\prime}$ 8	Quad.
Haro 1-14	591	12 $.\!\!^{\prime\prime}$ 9

Source LaTeX | All tables | In the text

	1 Introduction
	2 Imaging
	3 Spectroscopy
	4 Discussion
	5 Summary
	References