Table 1
Sample of stars and stellar properties.
| Source | Right Ascension | Declination | Spect. Type | Effective Temp. | Stellar Lum. | Stellar Mass | Age | UV flux |
| (°,′,′′), (J2000.0) | (h, m, s) (J2000.0) | (K) | (L⊙) | (M⊙) | (Myr) | (χ0) | ||
|
|
||||||||
| LkCa 15 | 04:39:17.78 | 22:21:03.34 | K5 | 4350 | 0.74 | 1.01 ± 0.02 | 3–5 | 2550 |
| DM Tau | 04:33:48.73 | 18:10:09.89 | M1 | 3720 | 0.25 | 0.53 ± 0.03 | 5 | 410 |
| MWC 480 | 04:58:46.26 | 29:50:36.87 | A4 | 8460 | 11.5 | 1.83 ± 0.05 | 7 | 8500 |
| GO Tau | 04:43:03.05 | 25:20:18.8 | M0 | 3850 | 0.37 | 0.5 | 3 | 410 |
Notes. Coordinates come from Piétu et al. (2006). Columns 3–7 are the spectral type, effective temperature, stellar luminosity, mass (Piétu et al. 2007 for DM Tau, MWC480, and LkCa15), and age (Simon et al. 2000). In Col. 8, the stellar UV luminosities (in units of the Draine 1978 interstellar UV field) are taken from Bergin et al. (2004) (LkCa 15 and DM Tau) or computed from the Kurucz (1993) ATLAS9 of stellar spectra (MWC 480 and GO Tau) for a distance of 100 AU from the star. Half of this flux is supposed to scatter downwards inside the disk.
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