Revisiting the cycle-rotation connection for late-type stars

Open Access

Table 1.

Sample of used object and results.

Name	B − V	S_MWO	Ref		T_eff	[Fe/H]	Age	d_cz	P_rot [d]	Ref	τ_c [d]	Ro	[yr]	Ref	Cal. [yr]		[yr]	Ref	Cal. [yr]
Sun	0.642	0.169	E17	−5.05	5777	0.00	4.6^a	0.292	25.4±1.0	B17	33.94	0.748	11.0±2.0	B17	10.3	0.06	88.0	P21	103.5	−0.18
HD 1835	0.659	0.349	B95	−4.30	5720	0.20	0.5^a	0.285	7.8±0.6	B17	37.18	0.210					9.1±0.3	B17	5.0	0.45
HD 3651	0.85	0.176	B95	−5.10	5211	0.13	7.1^a	0.324	44.0	B17	61.18	0.719	13.8±0.4	B17	11.7	0.15
HD 4628	0.89	0.23	B95	−4.81	5120	−0.27	5.3^a	0.306	38.5±2.1	B17	65.19	0.591	8.6±0.1	B17	9.9	−0.15
HD 10476	0.836	0.198	B95	−4.93	5244	−0.04	4.9^a	0.315	35.2±1.6	B17	59.83	0.588	9.6±0.1	B17	9.2	0.04
HD 10780	0.804	0.28	B95	−4.57	5321	0.03	2.3^a	0.301	22.14±0.55	O18	56.87	0.389	7.53±0.16	O18	5.6	0.25
HD 16160	0.918	0.226	B95	−4.86	5060	−0.12	7.5^a	0.309	48.0±4.7	B17	68.16	0.704	13.2±0.2	B17	12.4	0.06
HD 16673	0.524	0.215	B95	−4.65	6183	−0.01	0.8^a	0.196	5.7	N84	18.02	0.316	0.847±0.006	M19a	0.9	−0.07
HD 17051	0.561	0.225	BS18	−4.61	6045	0.15	1.0^a	0.239	8.5±0.1	B17	21.98	0.387	1.6	B17	1.4	0.13
HD 18256	0.471	0.185	B95	−4.86	6395	0.05	3.2^a	0.145	3.65±0.03	O18	13.56	0.269					6.64±0.06	O18
HD 20630	0.681	0.366	B95	−4.28	5654	0.06	0.6^a	0.279	9.2±0.3	B17	41.83	0.220					5.6±0.1	B17	6.4	−0.14
HD 22049	0.881	0.496	B95	−4.25	5140	−0.09	0.6^a	0.306	11.1±0.1	B17	64.27	0.173	2.9±0.1	B17	2.6	0.12	12.7±0.3	B17	8.5	0.33
HD 26965	0.82	0.206	B95	−4.87	5282	−0.29	7.2^a	0.299	43.0	B17	58.33	0.737	10.1±0.1	B17	11.5	−0.14
HD 30495	0.632	0.297	B95	−4.40	5804	0.09	1.1^a	0.268	11.4±0.2	B17	32.16	0.354	1.7±0.3	B17	1.6	0.06	12.2±3.0	B17	16.0	−0.31
HD 32147	1.049	0.286	B95	−4.85	4801	0.30	6.4^a	0.336	48.0	B17	83.93	0.572	11.1±0.2	B17	11.7	−0.06
HD 37394	0.84	0.453	B95	−4.27	5234	0.09	0.6^a	0.300	10.78±0.02	M17a	60.21	0.179					5.83±0.08	O18	8.4	−0.44
HD 43587	0.61	0.156	B95	−5.23	5876	−0.03	4.2^a	0.271	22.6±1.9	F20	28.58	0.791	10.44±3.03	F20	10.4	0.0
HD 75332	0.549	0.279	B95	−4.40	6089	0.10	0.4^a	0.223	4.8	M19a	20.60	0.233	0.493±0.003	M19a	0.5	−0.04
HD 75732	0.869	0.176	B22	−5.12	5167	0.34	5.2^a	0.334	37.4±0.5	M17a	63.05	0.593	10.9	B22	9.7	0.11
HD 76151	0.661	0.246	B95	−4.57	5714	0.11	1.6^a	0.285	15.0	B17	37.58	0.399	2.5±0.1	B17	2.4	0.02
HD 78366	0.585	0.248	B95	−4.52	5961	0.03	1.1^a	0.243	9.7±0.6	B17	24.99	0.388					12.2±0.4	B17	8.9	0.27
HD 100180	0.57	0.165	B95	−5.09	6013	0.00	2.3^a	0.243	14.0	B17	23.06	0.607	3.6±0.1	B17	3.4	0.06	12.9±0.5	B17	20.4	−0.58
HD 100563	0.48	0.202	B95	−4.72	6357	0.09	2.3^a	0.157	7.73±0.04	M19a	14.23	0.543	0.609±0.009	M19a
HD 103095	0.754	0.188	B95	−4.93	5449	−1.35	4.6^a	0.228	31.0	B17	52.52	0.590	7.3±0.1	B17	(9.6)	−0.32
HD 114710	0.572	0.201	B95	−4.75	6006	0.06	1.8^a	0.243	12.3±1.1	B17	23.31	0.528					16.6±0.6	B17	15.6	0.06
HD 115404	0.926	0.535	B95	−4.25	5043	−0.16	1.4^a	0.300	18.5±1.3	B17	69.03	0.268					12.4±0.4	B17	14.5	−0.17
HD 120136	0.508	0.191	B95	−4.81	6245	0.28	0.4^a	0.195	3.05±0.01	M17b	16.54	0.184	0.333±0.002	M17b	0.3	0.04
HD 128620	0.71	0.162	BS18	−5.16	5570	0.22	2.9^a	0.295	22.5±5.9	B17	48.88	0.460					19.2±0.7	B17	19.8	−0.03
HD 128621	0.9	0.209	BS18	−4.92	5098	0.24	4.7^a	0.329	36.2±1.4	B17	66.24	0.547	8.1±0.2	B17	9.2	−0.14
HD 140538	0.684	0.228	M19b	−4.66	5645	0.05	2.7^a	0.280	20.71±0.32	M19b	42.51	0.487	3.88±0.02	M19b	4.5	−0.16
HD 146233	0.652	0.171	M16	−5.03	5741	0.04	3.5^a	0.286	22.7±0.5	B17	35.81	0.634	7.1	B17	7.2	−0.02
HD 149661	0.827	0.339	B95	−4.44	5265	0.04	2.0^a	0.301	21.1±1.4	B17	58.98	0.358	4.0±0.1	B17	5.3	−0.32	17.4±0.7	B17	17.5	−0.01
HD 152391	0.749	0.393	B95	−4.28	5462	−0.02	0.8^a	0.294	11.4±1.4	B17	52.11	0.219					10.9±0.2	B17	9.3	0.15
HD 156026	1.144	0.77	B95	−4.37	4633	−0.18	1.4^a	0.311	21.0	B17	97.60	0.215					21.0±0.9	B17
HD 160346	0.959	0.3	B95	−4.66	4975	−0.02	4.4^a	0.320	36.4±1.2	B17	72.75	0.500	7.0±0.1	B17	9.0	−0.29
HD 165341 A	0.86	0.392	B95	−4.38	5188	0.07	1.7^a	0.305	19.9	B17	62.16	0.320	5.1±0.1	B17	4.9	0.04	15.5±0.0	B17	16.2	−0.04
HD 166620	0.876	0.19	B95	−5.02	5151	−0.18	6.4^a	0.306	42.4±3.7	B17	63.76	0.665	15.8±0.3	B17	11.1	0.3
HD 185144	0.786	0.215	B95	−4.79	5366	−0.22	3.5^a	0.299	27.7±0.77	O18	55.26	0.501	6.66±0.05	O18	7.3	−0.09
HD 190406	0.6	0.194	B95	−4.81	5910	0.05	1.9^a	0.252	13.9±1.5	B17	27.09	0.513	2.6±0.1	B17	2.6	−0.02	16.9±0.8	B17	16.0	0.06
HD 201091	1.069	0.658	B95	−4.30	4764	−0.16	3.7^a	0.314	35.4±9.2	B17	86.64	0.409	7.3±0.1	B17	8.3	−0.14
HD 201092	1.309	0.986	B95	−4.52	4366	−0.15	3.4^a	0.324	37.8±7.4	B17	126.86	0.298	11.7±0.4	B17
HD 219834 B	0.92	0.204	B95	−4.97	5055	0.21	6.2^a	0.329	43.0	B17	68.38	0.629	10.0±0.2	B17	11.0	−0.1
KIC 8006161	0.84	0.194	BS18	−4.96	5234	0.29	3.6^a	0.324	29.8±3.1	B17	60.21	0.495	7.4±1.2	B17	7.7	−0.04
KIC 10644253	0.59	0.219	S16	−4.65	5943	0.12	1.3^a	0.258	10.9±0.9	B17	25.67	0.425	1.5±0.1	B17	1.8	−0.19

Notes. Here, the used objects are listed with the corresponding B − V values from ESA (1997), except for the Sun. The solar B − V-value is taken from Cayrel de Strobel (1996). Furthermore, we are listed the both activity indicators Mount Wilson S-index (S_MWO) with the reference and the corresponding (Mittag et al. 2013) for each object, the effective temperature calculated with B − V relation from Gray (2005, Eq. (14.17)), the computed age with from the age relation by Mamajek & Hillenbrand (2008, label a: Eqs. (12)–(14) & label b: Eq. (3)), except the Sun, the solar age is taken from Bouvier & Wadhwa (2010, label c), and the median metalicity [Fe/H] from the catalogue by Soubiran et al. (2016, Version 2020-01-30), d_cz the relative depth of the convection zone based on the R_cz/R_⋆ from catalogue by van Saders & Pinsonneault (2012), the rotational period (P_rot) and with the corresponding reference, the convective turnover time (τ_c) calculated with the relation of Mittag et al. (2018) and the corresponding the Rossby number (Ro), the cycle on the short period cycle branch period () with reference, calculated cycle period (Cal. ), the ratio of the difference between calculated and measured short period cycle, the cycle period () on the long period cycle branch and the corresponding reference, calculated cycle period (Cal. ) and the ratio of the difference between calculated and measured long period cycle. The calculated cycle value for HD 103095 listed in parentheses is computed with Eq. (14) and the corresponding parameter given in Table 5.

References. (B95) Baliunas et al. (1995), (B22) Baum et al. (2022), (B17) Brandenburg et al. (2017), (BS18) Boro Saikia et al. (2018), (E17) Egeland et al. (2017), (F20) Ferreira et al. (2020), (M16) Mittag et al. (2016), (M17a) Mittag et al. (2017b), (M17b) Mittag et al. (2017a), (M19a) Mittag et al. (2019a), (M19b) Mittag et al. (2019b), (N84) Noyes et al. (1984a), (O18) Olspert et al. (2018), (P21) Ptitsyna & Demina (2021), (S16) Salabert et al. (2016), (V14) Vidotto et al. (2014).

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