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Table 1

Taurus disk sample.

(1) (2) (3) (4) (5) (6) (7) (8) (9) (10) (11)
Source RA Dec F 1.3mm Δn 10 μm M Sp. HαEW L bol L X
name (J2000) (J2000) [mJy]   strength [M] type [] [L] [1030 erg s-1]

Our subsample with new molecular line observations presented here
CW Tau 04:14:17.00  +28:10:57.8 96  ±  8 0.96 0.16 1.06 K3 135 1.35 2.844
CY Tau 04:17:33.72  +28:20:46.8 133  ±  11 0.50 0.12 0.55 M1.5 70 0.47 0.163
FT Tau 04:23:39.18  +24:56:14.3 130  ±  14 0.31 0.43 M3  >0.38 0.799
DG Tau 04:27:04.70  +26:06:16.2 443  ±  20 0.44 0.00 0.67 K6 113 0.90  <0.766
IQ Tau 04:29:51.56  +26:06:44.8 87  ±  11 0.40 0.35 0.68 M0.5 8 0.65 0.416
V806 Tau 04:32:15.41  +24:28:60.0 124  ±  13 1.46 0.35 M0 88 1.30
UZ Tau 04:32:42.96  +25:52.31.1 172  ±  15 0.58 0.45 0.18 M1-2 82 1.06 0.890
CI Tau 04:33:52.01  +22:50:30.1 190  ±  17 0.93 0.54 0.77 K7 102 0.87 0.195
DN Tau 04:35:27.37  +24:14:59.6 84  ±  13 0.33 0.22 0.70 M0 12 0.91 1.155
DO Tau 04:38:28.58  +26:10:49.9 136  ±  11 0.64 0.18 0.70 M0 100 1.20  <0.270
GO Tau 04:43:03.08  +25:20:18.6 83  ±  12 0.97 0.40 0.71 M0 81 0.27 0.249
DQ Tau 04:46:53.06  +17:00:00.2 91  ±  9 0.19 0.14 0.43 M0 113 0.91
DR Tau 04:47:06.22  +16:58:42.9 159  ±  11 0.61 0.27 0.38 K5 87 3.00

Sources with molecular line data already in the literature (see Table  4 )
V892 Tau 04:18:40.62  +28:19:15.5 289  ±  13 –1.22 0.65 B9 13 20.90 8.576
RY Tau 04:21:57.41  +28:26:35.6 229  ±  17 0.46 1.36 1.63 K0 20 7.60 5.520
T Tau 04:21:59.43  +19:32:06.4 280  ±  9 1.19 –0.10 K7 60 15.50 8.048
GG Tau 04:32:30.41  +17:31:40.2 593  ±  53 0.74 0.64 1.55 K7 54 1.55 0.160
DL Tau 04:33:39.06  +25:20:38.2 230  ±  14 0.24 0.09 0.70 K7 105 0.70  <1.000
DM Tau 04:33:48.73  +18:10:10.0 109  ±  13 1.93 0.96 0.25 M1.5 139 0.25  <0.457
AA Tau 04:34:55.42  +24:28:53.2 88  ±  9 0.50 0.35 0.78 K7 37 0.74 0.690
GM Aur 04:38:21.34  +26:09:13.7 253  ±  12 3.19 1.19 1.00 K7 96 1.00 1.241

Notes. Columns. 1–3: source name and 2MASS coordinates; Col. 4: 1.3 mm continuum fluxes from Beckwith (1996); Cols. 5−6: dust settling parameters Δn and the 10 μm silicate strength from Furlan et al. (2006); Col. 7: stellar masses from White & Ghez (2001) or Hartigan et al. (1995); Col. 8: spectral types from Luhman et al. (2010) or Rebull et al. (2010); Col. 9: Hα equivalent widths from Herbig & Bell (1988); Col. 10: bolometric luminosities from Palla & Stahler (2002), except for DQ Tau and DR Tau, which come from Kenyon & Hartmann (1995); Col. 11: X-ray luminosities from Güdel et al. (2007) or Damiani et al. (1995).

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