Table 1: Spectral properties for CBSS and V Sge stars with known orbital periods.

Source		 Type P $_{\rm orb}$ High/low Emission Absorption $-W{_\lambda}$(He II) i FWHM $\Delta v$ jet Refs.a
    (days) states jets (km s-1) jets (km s-1) (Å) ( $\hbox{$^\circ$ }$) (km s-1) (km s-1)  

RX J0537.7-7034		 CBSS 0.145 ... ... ... 2.9-4.8 45-70 ... ... 1
1E0035.4-7230 CBSS 0.171 ... ... ... 2.6 20-50 700 ... 2
V617 Sgr V Sge 0.207 y 780 ... 35-113 72 710-2900 $\sim$600 3, 4
WX Cen V Sge 0.416 ... 3500 -2900 12-37 55 700-1100 ... 5, 6
CAL 87 CBSS 0.442 ... ... ... 14 77 790 ... 7, 8
V Sge V Sge 0.514 y ... ... 46-117 71 700 ... 9, 10
QR And CBSS 0.660 y 815 -700 14 56 470-650 400 11, 12
RX J0513.9-6951 CBSS 0.762 y 3900 -3458 22 15 370 ... 13
CAL 83 CBSS 1.041 y ... ... 12 20-30 350 ... 13
MR Vel CBSS 4.028 ... 5200 ... 5.3 30-40 330-650 ... 14
a References: 1- Greiner et al. (2000); 2- van Teeseling et al. (1998); 3- Steiner et al. (1999); 4- Steiner et al. (2006); 5- Diaz & Steiner (1995); 6- Oliveira & Steiner (2004); 7- Hutchings et al. (1998); 8- Schandl et al. (1997); 9- Herbig et al. (1965); 10- Smak et al. (2001); 11- McGrath et al. (2001); 12- Deufel et al. (1999); 13- Cowley et al. (1998); 14- Motch (1998).

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