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Table 4

Derived inclinations.

Source PA i PACO iCO
° ° ° °

BP Tau 107 ± 5 39 ± 3  −119 ± 2 33 ± 6
CI Tau 285 ± 5 55 ± 5 285 ± 1 44 ± 3
CQ Tau  −37 ± 19  −31 ± 10  −36 ± 1  −29 ± 2
CY Tau 63 ± 5 34 ± 3 63 ± 1 28 ± 5
DG Tau 60 ± 4 32 ± 2 43 ± 2 38 ± 2
DG Tau b 114 ± 1 64 ± 2 117 ± 3  > 75
DL Tau 141 ± 3 38 ± 2 144 ± 3 43 ± 3
DM Tau 67 ± 5  −36 ± 3 63 ± 1  −34 ± 1
FT Tau 31 ± 14 21 ± 5 29 ± 4 23 ± 14
GM Aur 139 ± 3 54 ± 3 144 ± 1 50 ± 1
HL Tau 42 ± 2 45 ± 1 45 45
LkCa 15 150 ± 2 48 ± 2 150 ± 1 52 ± 1
MWC 480 75 ± 5 30 ± 2 58 ± 1 37 ± 1
MWC 758 147 ± 292  −11 ± 249 141 ± 1 18 ± 36
UZ Tau E  −3 ± 3 131 ± 2  −4 ± 2 124 ± 2
UZ Tau W  −34 ± 14 124 ± 12  −4 ± 2 124 ± 2
HH 30 35 ± 1 98 ± 1 32 ± 3 99 ± 3

Notes. Position angles are those of the disk rotation axis. The inclinations iCO have been derived from CO observations except for UZ Tau W (assumed to be equal to that of UZ Tau E), DG Tau, and DG Tau-b, which come from Eislöffel & Mundt (1998). For HL Tau, the CO outflow defines iCO and PACO. Conventions for PA and i use the rotation axis orientation as described by Piétu et al. (2007).

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