Table 1
Stellar properties.
RA | Dec | Teff | J a | A J | Dist | L bol | M ∗ | ||||||||
Target | 2MASS ident | (J2000) | (J2000) | SpT | (K) | (mag) | (mag) | (pc) | (10-3L⊙) | (M⊙) | Ref. | ||||
|
|||||||||||||||
Our sample | |||||||||||||||
2M04152746 | J04155799+2746175 | 04 | 15 | 57.994 | +27 | 46 | 17.57 | M5.5 | 3054 | 11.745 | 0.16 | 140 | 60 | 0.14 | 1, 5 |
2M04232801 | J04230607+2801194 | 04 | 23 | 06.07 | +28 | 01 | 19.5 | M6 | 2990 | 12.242 | 0.21 | 140 | 39 | 0.096 | 2 |
2M04332615 | J04334465+2615005 | 04 | 33 | 44.652 | +26 | 15 | 00.53 | M4.75 | 3161 | 11.639 | 0.85 | 140 | 125 | 0.20 | 1 |
2M04412534 | J04414825+2534304 | 04 | 41 | 48.250 | +25 | 34 | 30.50 | M7.75 | 2763 | 13.730 | 0.28 | 140 | 10 | 0.036 | 2, 5 |
CFHT-6 | J04390396+2544264 | 04 | 39 | 03.960 | +25 | 44 | 26.42 | M7.25 | 2846 | 12.646 | 0.11 | 140 | 23 | 0.050 | 2, 5 |
CFHT-18 | J04292165+2701259 | 04 | 29 | 21.653 | +27 | 01 | 25.95 | M5.25 | 3089 | 10.801 | 0b | 140 | 130 | 0.16 | 2 |
CIDA-1 | J04141760+2806096 | 04 | 14 | 17.609 | +28 | 06 | 09.70 | M5.5 | 3054 | 11.726 | 0.79 | 140 | 106 | 0.14 | 2, 5 |
GM Tau | J04382134+2609137 | 04 | 38 | 21.340 | +26 | 09 | 13.74 | M6.5 | 2935 | 12.804 | 0.037 | 140 | 19 | 0.075 | 2 |
ISO-Oph 32 | J16262189−2444397 | 16 | 26 | 21.899 | −24 | 44 | 39.76 | M8 | 2710 | 12.340 | 0.00 | 130 | 23 | 0.030 | 3 |
ISO-Oph 102 | J16270659−2441488 | 16 | 27 | 06.596 | −24 | 41 | 48.84 | M5.5 | 3054 | 12.433 | 0.13 | 130 | 27 | 0.14 | 3 |
ISO-Oph 160 | J16273742−2417548 | 16 | 27 | 37.422 | −24 | 17 | 54.87 | M6 | 2990 | 14.148 | 1.70 | 130 | 21 | 0.096 | 4 |
|
|||||||||||||||
Literature sample | |||||||||||||||
L1521F-IRSc | 04 | 28 | 38.95 | +26 | 51 | 35.1 | M6−M8 | ~2880 | ... | ... | 140 | ... | 0.058 | 6, 8 | |
FW Tau A+B+C | J04292971+2616532 | 04 | 29 | 29.710 | +26 | 16 | 53.21 | M5.5 | 3054 | 10.340 | 0.00 | 140 | 190 | 0.14 | 6, 8 |
FN Tau | J04141458+2827580 | 04 | 14 | 14.590 | +28 | 27 | 58.06 | M5 | 3125 | 9.469 | 0.00 | 140 | 432 | 0.18 | 6, 8 |
CFHT 12 | J04330945+2246487 | 04 | 33 | 09.457 | +22 | 46 | 48.70 | M6 | 2990 | 13.154 | 0.45 | 140 | 21 | 0.096 | 6, 8 |
ZZ Tau IRSc | J04305171+2441475 | 04 | 30 | 51.714 | +24 | 41 | 47.51 | M5 | 3125 | 12.842 | 0.82 | 140 | 40 | 0.18 | 6, 8 |
J04381486+2611399c | J04381486+2611399 | 04 | 38 | 14.861 | +26 | 11 | 39.94 | M7.25 | 2846 | 15.176 | 0.26 | 140 | 2.6 | 0.050 | 6, 8 |
CIDA 7 | J04422101+2520343 | 04 | 42 | 21.017 | +25 | 20 | 34.38 | M4.75 | 3161 | 11.397 | 0.32 | 140 | 98 | 0.20 | 6, 8 |
KPNO-10 | J04174955+2813318 | 04 | 17 | 49.554 | +28 | 13 | 31.85 | M5 | 3125 | 11.889 | 0.34 | 140 | 63 | 0.18 | 6, 8 |
IRAS 04158+2805c | J04185813+2812234 | 04 | 18 | 58.138 | +28 | 12 | 23.49 | M5.25 | 3089 | 13.778 | 0.66 | 140 | 14 | 0.16 | 6, 8 |
J04202555+2700355 | J04202555+2700355 | 04 | 20 | 25.554 | +27 | 00 | 35.55 | M5.25 | 3089 | 12.861 | 0.42 | 140 | 27 | 0.16 | 6, 8 |
KPNO-3 | J04262939+2624137 | 04 | 26 | 29.392 | +26 | 24 | 13.79 | M6 | 2990 | 13.323 | 0.42 | 140 | 17 | 0.096 | 6, 8 |
MHO-6 | J04322210+1827426 | 04 | 32 | 22.109 | +18 | 27 | 42.64 | M4.75 | 3161 | 11.711 | 0.37 | 140 | 77 | 0.20 | 6, 8 |
CFHT 4 | J04394748+2601407 | 04 | 39 | 47.484 | +26 | 01 | 40.78 | M7 | 2880 | 12.168 | 0.00 | 140 | 33 | 0.058 | 6, 8 |
ESO-HA 559 | J11062554−7633418 | 11 | 06 | 25.549 | −76 | 33 | 41.87 | M5.25 | 3089 | 13.009 | 1.01 | 160 | 52 | 0.16 | 7 |
2M0444+2512 | J04442713+2512164 | 04 | 44 | 27.132 | +25 | 12 | 16.41 | M7.25 | 2846 | 12.195 | 0.026 | 140 | 33 | 0.050 | 6, 8 |
TWA 30Bd | J11062554−7633418 | 11 | 32 | 18.223 | −30 | 18 | 31.65 | M5 | 3125 | 15.350 | 0.00 | 46 | 0.2 | 0.12 | 9 |
TWA 32 | J12265135−3316124 | 12 | 26 | 51.365 | −33 | 16 | 12.55 | M6 | 2990 | 10.691 | 0.00 | 59 | 23 | 0.072 | 9 |
TWA 34 | J12265135−3316124 | 10 | 28 | 45.808 | −28 | 30 | 37.46 | M5 | 3125 | 10.953 | 0.00 | 47 | 12 | 0.12 | 9 |
Notes.
J-band magnitude from 2MASS (Cutri et al. 2003; Skrutskie et al. 2006).
Zero extinction is assumed owing to the lack of better estimates. Previous measurements, e.g., AJ = 2 mag by Luhman et al. (2009) have likely been corrupted by its binarity.
These targets were classified as likely Class I in Sect. 3.1 and are excluded from all disk analysis.
TWA 30B likely has an edge-on disk (Looper et al. 2010).
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