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).
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.