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Table 3

Very young stars and PMS candidates selected from the lithium content.

# Name RasTyc α (2000) Δ (2000) Sp. Type Teff logg [Fe/H] A(Li)
h m s °  ′′ (ct/s) (K) (dex) (dex)
#1 BD+78 853 0000+7940 00 00 41.14 +79 40 39.9 0.106 G2V 5738 4.19 –0.03 3.28 –4.43
#2 TYC 4496-780-1†,‡ 0013+7702 00 13 40.52 +77 02 10.9 0.102 G0V 5924 4.14 –0.03 3.31 –3.33
#3 TYC 4500-1478-1 0038+7903 00 38 06.03 +79 03 20.7 0.133 K1V 5160 4.30 –0.06 3.24 –3.87
#4 BD+78 19†,⋆ 0039+7905 00 39 40.13 +79 05 30.8 0.077 G5V 5444 4.14 –0.11 3.05 –4.57
#5 TYC 3266-1767-1 0046+4808 00 46 53.09 +48 08 45.2 0.278 K2V 5067 4.21 –0.09 3.58 –4.02
#6 BD+49 646 0222+5033 02 22 33.82 +50 33 37.8 0.491 K2V 5094 4.27 –0.12 2.84 –3.90
#7 TYC 3695-2260-1 0230+5656 02 30 44.81 +56 56 13.0 0.051 G1V 5874 4.31 –0.03 3.46 –4.47
#8 TYC 2338-35-1 0252+3728 02 52 24.71 +37 28 52.0 0.048 G1.5V 5784 4.35 0.02 4.02 –4.44
#9 TYC 4321-507-1 0300+7225 03 00 14.67 +72 25 41.4 0.084 K2V 5079 4.59 –0.01 2.94 –4.00
#10 Cl Melotte 20 94 0311+4810 03 11 16.82 +48 10 36.9 0.092 G1.5V 5856 4.35 0.02 3.39 –4.24
#11 TYC 3710-406-1 0316+5638 03 16 28.11 +56 38 58.1 0.084 K1V 5208 4.50 –0.05 2.81 –4.18
#12 TYC 3715-195-1 0323+5843 03 23 07.08 +58 43 07.4 0.148 K1V 5212 4.48 –0.07 2.97 –3.92
#13 Cl Melotte 20 935 0331+4859 03 31 28.98 +48 59 28.6 0.081 G1.5V 5816 4.30 –0.10 3.24 –4.05
#14 TYC 2876-1944-1 0359+4404 03 59 16.70 +44 04 17.1 0.264 K1V 5235 4.50 –0.06 3,36 –3.62
#15 TYC 3375-720-1 0616+4516 06 16 46.95 +45 16 03.1 0.097 G2V 5739 4.21 0.11 3.47 –3.83
#16 TYC 3764-338-1 0621+5415 06 21 56.92 +54 15 49.0 0.426 G2V 5719 4.14 –0.08 2.98 –4.15
#17 HD 234808* 1908+5018 19 08 14.03 +50 18 49.6 0.045 G8III-IV 5223 3.39 –0.37 3.69 –4.20
#18 KIC 8429280 1925+4429 19 25 01.98 +44 29 50.7 0.254 K2V 5055 4.41 –0.02 2.96 –3.96
#19 BD-03 4778 2004−0239 20 04 49.35 − 02 39 19.7 0.175 K1V 5183 4.39 –0.02 3.33 –4.26
#20 HD 332091 2016+3106 20 16 57.83 +31 06 55.6 0.167 K1V 5087 4.57 0.01 2.88 –3.72
#21 TYC 2694-1627-1 2036+3456 20 36 16.87 +34 56 46.1 0.037 G1V 5832 4.33 –0.01 3.30 –4.33
#22 TYC 2178-1225-1 2039+2644 20 39 40.81 +26 44 48.4 0.227 K1V 5149 4.30 –0.08 2.80 –4.19
#23 BD+68 1182 2106+6906 21 06 21.74 +69 06 41.0 0.114 G1.5V 5828 4.31 –0.01 3.39 –4.31
#24 TYC 3589-3858-1 2120+4636 21 20 55.42 +46 36 12.4 0.142 G1.5V 5699 4.36 0.04 3.07 –4.29
#25 BD+76 857a 2223+7741 22 23 18.87 +77 41 57.7 0.114 G1.5V 5745 4.29 –0.04 3.60 –4.28
#26 TYC 1154-1546-1 2233+1040 22 33 00.37 +10 40 34.3 0.053 G1.5V 5544 4.39 0.03 3.65 –3.44
#27 HD 214995** 2241+1430 22 41 57.40 +14 30 59.2 0.094 K0III 4678 2.77 –0.04 3.61 –6.11
#28 BD+17 4799 2244+1754 22 44 41.49 +17 54 19.0 0.835 K1V 5161 4.41 –0.02 2.91 –4.14
#29 TYC 3992-349-1 2246+5749 22 46 13.19 +57 49 58.0 0.034 G2V 5752 4.32 –0.05 3.33 –4.31
#30 TYC 2751-9-1 2307+3150 23 07 24.83 +31 50 14.1 0.462 K4V 4774 4.58 0.05 2.48 –4.15
#31 V395 Cep 2320+7414 23 20 52.07 +74 14 07.1 0.035 K0IV 5093 3.58 –0.02 3.68 –3.27
#32 TYC 584-343-1 2321+0721 23 21 56.36 +07 21 33.0 0.067 K0V 5207 4.24 0.01 3.20 –4.25
#33 TYC 4606-740-1 2351+7739 23 51 17.29 +77 39 35.3 0.169 K1V 5146 4.52 –0.07 3.51 –3.84
a TYC 2282-1396-1 0106+3306 01 06 18.71 +33 06 01.9 0.161 G4V 5606 4.31 –0.14 3.11 –4.16
b BD+42 636 0249+4255 02 49 54.69 +42 55 27.1 0.036 G1.5V 5825 4.24 –0.02 3.07 –4.52
c TYC 3325-98-1 0344+5043 03 44 34.50 +50 43 47.5 0.074 K0V 5349 4.40 –0.06 3.01 –3.99
d TYC 2949-780-1 0646+4147 06 46 46.74 +41 47 12.2 0.043 G2V 5696 4.16 0.13 3.29 –4.60
e TYC 2087-1742-1 1731+2815 17 31 03.33 +28 15 06.1 0.305 K1V 5169 4.47 –0.02 2.91 –3.98
f KIC 7985370 1956+4345 19 56 59.73 +43 45 08.2 0.036 G1.5V 5815 4.24 –0.05 3.05 –4.50
g BD+35 4198 2038+3546 20 38 17.71 +35 46 33.3 0.058 G1.5V 5895 4.23 0.01 3.00 –4.86
h BD+39 4490 2114+3941 21 14 55.24 +39 41 11.9 0.099 G1.5V 5930 4.27 –0.02 3.01 –4.75
i TYC 3198-1809-1 2203+3809 22 03 49.83 +38 09 42.9 0.033 G5IV-V 5678 4.28 0.04 3.06 –4.95
j TYC 576-1220-1 2308+0000 23 08 50.46 +00 00 52.8 0.104 G2V 5620 4.38 –0.00 3.25 –3.91
k TYC 4283-219-1 2324+6215 23 24 40.37 +62 15 51.1 0.037 F9V 6011 3.97 –0.21 3.12 –4.84

Notes. () X-ray count rate from the second ROSAT all-sky survey source catalog (2RXS; Boller et al. 2016). (†) PMS star in Cepheus discovered by Guillout et al. (2010). (‡) Close visual pair (ρ = 1. ′′41, Δ V ≃ 2.2 mag; Fabricius et al. 2002). Parameters of the brighter component. (⋆) SB2 system composed of two nearly identical stars. Parameters derived from spectra taken close to the conjunctions. (∙) Very young star in the Kepler field discovered by Frasca et al. (2011). (◇) X-ray count rate from the ROSAT All-Sky Bright Source Catalog (1RXS; Voges et al. 1999). (⊙) Close visual pair (ρ = 0. ′′82, Δ V ≃ 0.15 mag; Fabricius et al. 2002). (⊕) Close visual pair (ρ = 0. ′′85, Δ V ≃ 0.29 mag; Fabricius et al. 2002). (⊗) Very young star in the Kepler field discovered by Fröhlich et al. (2012). (*) Discarded as PMS candidate on the basis of spectral classification and the position in the HR diagram. Likely lithium-rich giant. (**) Discarded as PMS candidate on the basis of spectral classification and the very low Hα flux. Lithium-rich giant.

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