Online Material
Table 4:
Parameters for YSOs in L1630N. Column 4: a the values estimated from our VIMOS spectra; b the values from Flaherty & Muzerolle (2008). Column 6: stellar bolometric luminosity derived from optical SED fitting (see Sect. 3.3.2). Column 9: classification based on the criteria in Appendix A. Column 11: aggregate/cluster population or distributed population. Columns 13-14: stellar masses and ages estimated using PMS evolutionary tracks from Dotter et al. (2008). Columns 16-18: accretion rates estimated with H
,
H
,
and He I 5876 Å emission line luminosities, respectively.
Table 5:
Parameters for YSOs in L1641. Column 4: a the values estimated from our VIMOS spectra; b the values from Allen (1995); c the values from Gâlfalk & Olofsson (2008). Column 6: stellar bolometric luminosity derived from optical SED fitting (see Sect. 3.3.2). Column 9: classification based on the criteria in Appendix A. Column 11: aggregate/cluster population or distributed population. Column 13-14: stellar masses and ages estimated using PMS evolutionary tracks from Dotter et al. (2008). Column 16-18: accretion rates estimated with H,
H,
and He I 5876Å emission line luminosities, respectively.
Table 6: Photometric magnitudes of YSOs in L1630N.
Table 7: Photometric magnitudes of YSOs in L1641.
Table 10: The equivalent widths of emission lines on the optical spectra for YSOs in L1630N.
Table 11: The equivalent widths of emission lines on the optical spectra for YSOs in L1641.
Table 16: Photometric magnitudes for transition disk object candidates.