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Table 4.

First five stars of the list of IC 4996 members with their classification and intrinsic parameters.

No. RA(J2000) Dec(J2000) V Sp. type AV (Y − V)0 V0 BC log Teff log L/L μα σ(μα) μδ σ(μα) d (pc) p
34 20:16:02.16 +37:41:30.1 15.929 a7 V 2.34 0.27 13.59 +0.02 3.903 1.004 −2.713 0.057 −5.625 0.066 1811 0.90
136 20:16:07.40 +37:42:34.6 14.442 a0 V 1.84 0.17 12.60 –0.25 3.982 1.508 −2.472 0.032 −5.226 0.033 1919 0.97
162 20:16:08.55 +37:35:08.2 13.662 b8 V 2.20 0.11 11.46 –0.80 4.107 2.184 −2.796 0.025 −5.186 0.027 1843 0.96
203 20:16:10.93 +37:34:53.1 14.948 a0 V 2.27 0.18 12.68 –0.20 3.978 1.456 −2.540 0.036 −5.469 0.037 2042 0.96
289 20:16:15.44 +37:40:15.4 15.135 a3 V 1.78 0.22 13.36 –0.03 3.949 1.116 −2.750 0.044 −5.411 0.046 2058 0.96

Notes. The last six columns give the proper motions from Gaia DR2, the estimated distances from Bailer-Jones et al. (2018), and the membership probability from GMM. The full table is available at the CDS.

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