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Table 1

Stellar properties of the sample studied.

Name α(h m s) δ(◦ ′ ′′) Distancea Spectral Type Ref. LXb
(J2000) (J2000) (pc) (erg s-1)

MHO 1 04:14:26.0 +28:06:04.2 140 M2.5 1 1.6 × 1030
MHO 2 04:14:26.4 +28:05:59.7 140 M2.5 1
V892 Tau 04:18:40.7 +28:19:12.3 140 B9 1 9.2 × 1030
CoKu Tau 1 04:18:51.6 +28:20:26.5 140 M0 1 ...
FS Tau A 04:22:02.2 +26:57:30.2 140 M0 2 3.2 × 1030
SST042936+243555 04:29:36.2 +24:35:52.5 140 M3 2 ...
XZ Tau 04:31:39.8 +18:13:57.3 140 M2 3 9.6 × 1029
L1551 IRS 5 04:31:34.2 +18:08:04.7 140  <K6 1 2.1 × 1028
UY Aur 04:51:47.9 +30:47:23.0 140 M0 3 2.6 × 1029
VZ Cha 11:09:24.4 –76:23:22.4 178 K7 4 2.5 × 1029
RXJ1111.7-7620 11:11:47.0 –76:20:10.8 163 K6 5 1.5 × 1030
V853 Oph 16:28:45.3 –24:28:18.9 125 M3.75 6 3.1 × 1030
IRS 60 16:31:31.0 –24:24:40.0 125 K2 4 2.6 × 1029
EC 92 18:29:57.8 +01:12:53.1 260 K7-M2 7 9.5 × 1030

Notes. 

(a)

Distance compiled in Güdel et al. (2010).

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