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Table 2

Parameters of late-type Carina members.

HSB2012 S / N RV vsini T eff A V Li EW γ log age Hα SB2
(km s-1) (km s-1) (K) (mÅ) (yr)
796 17.0 2.5 ± 2.5 20.3 ± 3.3 5694 ± 218 0.75 137.8 ±12.0 1.01 ± 0.015 ... Y N
800 43.1 −0.7±6.2 74.2 ± 8.1 5978 ± 95 0.81 105.3 ± 6.4 1.009 ± 0.006 ... Y N
908 62.5 −11.5 ± 7.4 30.0 ± 12.7 7541 ± 92 1.77 89.7 ± 3.9 0.999 ± 0.004 ... N N
907 28.5 −4.9 ± 0.6 13.6 ± 1.7 4869 ± 95 0.31 202.0 ± 6.6 0.969 ± 0.009 6.98 N N
954 49.6 −6.5 ± 8.0 69.0 ± 2.7 5727 ± 67 1.52 160.3 ± 6.3 1.01 ± 0.005 ... N N
953 25.9 −3.6 ± 1.4 24.8 ± 1.5 4865 ± 104 2.78 371.0 ± 8.3 1.022 ± 0.01 6.30 N N
995 16.6 −6.8 ± 2.0 13.0 ± 1.6 5019 ± 172 2.44 373.8 ± 11.0 0.999 ± 0.016 ... Y N
998 47.0 −9.3 ±7.0 92.4 ± 1.4 4942 ± 60 2.44 349.6 ± 7.4 1.011 ± 0.006 6.12 Y N
1035 130.4 −0.7 ± 15.1 99.4 ± 9.6 7498 ± 43 1.67 38.6 ± 2.3 0.998 ± 0.002 ... N N
1051 18.2 −5.2 ±2.0 15.0 ± 0.5 5177 ± 159 2.04 371.1 ± 7.9 1.028 ± 0.015 6.89 Y N

Notes. Column HSB2012 reports the identifier in Hur et al. (2012). S/N is the spectrum median signal/noise ratio. RV is the heliocentric radial velocity. Errors on Teff are statistical only. The gravity index γ is defined in Damiani et al. (2014). Column “log age” is the photometric age. Column Hα reports “Y” if an excess Hα emission is detected, either from accretion (CTTS) or chromospheric, distinct from the nebular Hα emission. Column “SB2” is “Y” for SB2 binaries. Full table is available at the CDS.

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