Theoretical values of convective turnover times and Rossby numbers for solar-like, pre-main sequence stars

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Table 3:

Rossby numbers and B-V for IC 2602 stars.
Name^a	B-V^a	Ro	Ro	Ro^a
Name^a	B-V^a	(Pur. Theor.)	(Semi-Theor.)	Ro^a
B134	0.95	0.0132	0.1767	0.110
W79	0.83	0.0176	0.2107	0.117
R15	0.93	0.0136	0.0967	0.059
R24A	1.43	0.0039	0.0127	0.013
R27	1.50	0.0023	0.0328	0.045
R29	1.11	0.0097	0.0440	0.031
R43	0.95	0.0132	0.0203	0.013
R52	1.07	0.0105	0.0084	0.006
R56	1.43	0.0039	0.0418	0.043
R58	0.65	0.0281	0.0355	0.015
R66	0.68	0.0261	0.1748	0.082
R70	0.69	0.0255	0.2212	0.107
R72	0.64	0.0288	0.0691	0.029
R77	1.47	0.0030	0.0855	0.104
R83	0.62	0.0303	0.1226	0.049
R88A	1.20	0.0080	0.0035	0.003
R89	1.24	0.0073	0.0757	0.059
R92	0.67	0.0267	0.1117	0.050
R93	1.37	0.0050	0.0802	0.075
R94	1.39	0.0047	0.0295	0.028
R95A	0.87	0.0154	0.0362	0.021
R96	1.25	0.0071	0.0282	0.022

^(a) Barnes et al. (1999).

Source LaTeX | All tables | In the text

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