Multiple and changing cycles of active stars - II. Results

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Table 1:

The stellar sample. I. Photometric observations.
Star	Rot. Per.^a	Sp. type	$v\sin i$	i	Time-base
	(days)		(km s^-1)	( $^\circ$ )	(years)
AB Dor	0.515	K0V	91	60	18
LQ Hya	1.601	K2V	27	65	25
V833 Tau	1.788	K5V	6.3	20	20
"	photographic + photometric data				109
V410 Tau	1.872	K4	74	70	34
EI Eri	1.947	G5IV	51	46	28
FK Com	2.400	G4III	155	60	28
V711 Tau	2.838	G5IV/K1IV	41	40	30
UZ Lib	4.768	K0III	67	50	17
UX Ari	6.437	G5V/K0IV	39	60	23
HU Vir	10.388	K1IV-III	25	65	17
IL Hya	12.905	K0III-IV	26.5	55	20
XX Tri	23.969	K0III	21	60	21
HK Lac	24.428	K0III	20	65	50
IM Peg	24.649	K2III-II	26.5	70	29

The stellar parameters are from Strassmeier (2002), and the references therein.
^a The orbital period is given in case of synchronised binary.

Source LaTeX | All tables | In the text

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