Table 1
Teff, log (g) and rotational velocities derived by comparison with models for the sample of sources observed with Magellan/MIKE.
Source | Mdl1 | SpT | Teff | log (g) | vsin(i) | Acc2 | log (Ṁacc) | Binary3 |
(K) | (km s-1) | (M⊙/yr) | ||||||
|
||||||||
LOri017* | Kur | – | 4250 | 4.0 | 70 | – | ||
LOri031 | Kur | M3.5 | 3750 | 4.0 | 40 | N | ||
LOri042 | Kur | M4.0 | 3750 | 4.0 | 30 | N | ||
LOri050 | NG | M4.0 | 3700 | 4.0 | 60 | Y | −10.878 ± 0.05 | M08, S08 |
LOri055 | NG | M4.0 | 3700 | 4.0 | <20 | N | ||
LOri056 | NG | M4.5 | 3700 | 4.0 | – | N | ||
LOri057 | NG | M5.5 | 3700 | 4.0 | <20 | N | ||
LOri058 | NG | M3.5 | 3500 | 4.0 | – | N | ||
LOri059 | NG | M4.5 | 3500 | 4.0 | – | N | ||
LOri060 | NG | M4.0 | 3500 | 4.0 | 20-40 | N | ||
LOri063 | NG | M4.0 | 3700 | 4.0 | – | Y | ||
LOri068 | NG | M4.5 | 3700 | 4.0 | – | N | ||
LOri073 | NG | M5.0 | 3700 | 4.0 | – | N | ||
LOri075 | NG | M5.0 | 3400 | 4.0 | 65 | N | M08, B11 |
Notes. We also display other relevant information about the sources such as accretion rate (derived in this work) or binarity.
There were problems with the extraction of several orders. We used the Teff corresponding to the SED fit provided in Paper I.
Y indicates that the object fulfills the accretion criterion by Barrado y Navascués & Martín (2003) (those marked with N do not).
Binary system according to Maxted et al. (2008, M08), Sacco et al. (2008, S08) or this work (B11).
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