Activity trends in young solar-type stars | Astronomy & Astrophysics (A&A)

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Table 5

Rotation periods, activity indices, age estimates and identifications of kinematic group membership for the sample stars from previous studies.


Star	P_rot [d]		log R_X	Age^a [Myr]	Group^b	Star	P_rot [d]		log R_X	Age^a [Myr]	Group^b


HD 1405	1.745¹	–3.85²⁶	...	T_iso: 20²	AB^3,48,49,50	HD 82558	1.6009¹¹	–3.66²⁹	–3.03²⁹	T_X: 80²⁹	IC⁵¹
	1.76159²			T_iso: 30–80⁴⁵	LA⁴⁶		1.6603¹⁴	–4.03³⁷	–3.06⁴³
	1.76³						1.5978¹⁵	–3.63³⁹	–3.17⁴⁴
HD 10008	7.15⁴	–4.2⁴	–4.48⁶	T_gyro: 211⁴	HLA⁴⁹		1.60114¹⁶
		–4.38⁶	–4.43²⁹	T_HK: 360²⁸	LA^29,46		1.6007¹⁷
		–4.530²⁷		T_HK: 130²⁹	TWA⁵¹		1.6043¹⁸
		–4.427²⁸		T_X: 440²⁹			1.60514¹⁹
		–4.29²⁹				HD 116956	7.80⁶	–4.22⁴¹	–4.48⁶	T_HK: 260²⁸	LA^6,29,46
		–4.45³⁰					7.8288²⁰	–4.447²⁷	–4.36²⁹	T_HK: 70⁴¹	TWA⁵¹
		–4.41³¹						–4.385²⁸	–4.35³⁵	T_X: 360⁴⁶
HD 26923	...	–4.52⁶	–4.64⁶	...	UMa^6,46,51			–4.22³⁵
		–4.503⁹	–4.41³⁵			HD 128987	9.35⁶	–4.451²⁸	–4.78⁶	T_HK: 430²⁸	IC²⁹
		–4.555²⁷						–4.51²⁹	–4.86²⁹	T_HK: 650²⁹
		–4.496³²						–4.45³⁰		T_X: 680²⁹
		–4.49³³						–4.439³⁴
		–4.521³⁴				HD 130948	7.85⁶	–4.45⁶	–4.69⁶	T_HK: 380²⁸	...
		–4.39³⁵						–4.434²⁸	–4.65²⁹	T_HK: 190²⁹
HD 29697	3.936⁵	–4.066²⁷	–3.25³⁵	...	UMa⁴⁶			–4.34²⁹	–4.50³⁵	T_HK: 870³⁶
		–4.06³⁵						–4.64³⁵		T_X: 330²⁹
HD 41593	7.97⁶	–4.36⁶	–4.59⁶	T_HK: 320^28,36	UMa^6,46,51			–4.50³⁶
		–4.456²⁷						–4.45⁴²
		–4.409²⁸				HD 135599	5.97⁶	–4.663²⁷	–4.94⁶	T_HK: 200²⁹	UMa⁶
HD 43162	7.24⁷	–4.40⁶	–4.31⁶	T_HK: 460²⁸	IC^29,51			–4.35²⁹	–5.11²⁹	T_HK: 950³⁶
		–4.460²⁸	–4.29²⁹	T_HK: 280²⁹				–4.52³⁵		T_X: 1340²⁹
		–4.39²⁹		T_HK: 370³⁶				–4.52³⁶
		–4.480³⁴		T_X: 280²⁹		HD 141272	14.045⁴	–4.2⁴	–4.62⁶	T_gyro: 773⁴	HLA⁵²
		–4.40³⁶					14.01⁶	–4.452²⁷	–4.40²⁹	T_HK: 420²⁸	LA^29,46
HD 63433	6.46⁶	–4.34⁶	–4.55⁶	T_HK: 170²⁸	UMa^6,46,51			–4.447²⁸	–4.40³⁵	T_HK: 200²⁹


		–4.424²⁷	–4.52³⁵	T_HK: 350³⁶				–4.35²⁹		T_HK: 340³⁶
		–4.331²⁸						–4.39³⁵		T_X: 430²⁹
		–4.39³⁵						–4.39³⁶
		–4.39³⁶						–4.49³⁹
HD 70573	3.296⁵	–4.187²⁸	...	T_HK: 50²⁸	HLA⁴⁹	HD 171488	1.338⁵	–4.21³⁷	–3.61⁴³	T_iso: 30²¹	LA⁴⁶
		–4.10³⁷			LA⁴⁶		1.3371²¹			T_iso: 50⁴⁷
HD 72760	...	–4.39⁶	–4.78⁶	T_HK: 200²⁸	Hya^29,46		1.313²²			T_Li: 50²¹
		–4.454²⁷	–4.76²⁹	T_HK: 440²⁹			1.337²³
		–4.350²⁸		T_HK: 310³⁶			1.3372²⁴
		–4.454²⁹		T_X: 690²⁹		HD 180161	5.49⁴	–4.6⁴	–4.67⁶	T_gyro: 127⁴	Hya^6,29,46
		–4.38³⁶					9.7⁶	–4.44⁶	–4.68²⁹	T_HK: 530²⁸
		–4.57³⁷						–4.481²⁸	–4.66³⁵	T_HK: 690²⁹
		–4.21³⁸						–4.52³⁶		T_HK: 950³⁶
HD 72760		–4.28³⁹				HD 180161		–4.52²⁹		T_X: 560²⁹
HD 73350	6.14⁶	–4.49⁶	–4.85⁶	T_HK: 1170²⁸	Hya^6,29			–4.52³⁵
	12.3⁸	–4.48⁸	–4.78²⁹	T_HK: 300²⁹		HD 220182	7.489⁴	–4.2⁴	–4.59⁶	T_gyro: 230⁴	...
		–4.657²⁷	–4.80⁴³	T_HK: 830³⁶			7.66⁶	–4.34⁶	–4.61²⁹	T_HK: 100²⁸
		–4.605²⁸		T_X: 460²⁹				–4.503²⁷	–4.58³⁵	T_HK: 40²⁹
		–4.40²⁹						–4.269²⁸		T_HK: 260³⁶
		–4.49³⁶						–4.15²⁹		T_X: 550²⁹
		–4.49⁴⁰						–4.37³⁵
HD 82443	5.409⁴	–4.22⁶	–4.01⁶	T_gyro: 130⁴	LA^29,46			–4.37³⁶
	5.43⁵	–4.211⁹	–3.93²⁹	T_HK: 20²⁹	Ple⁶	SAO 51891	2.42⁵	–4.05³⁷	...	...	LA⁴⁶
	5.42⁶	–4.0¹¹	–3.94³⁵	T_X: 220²⁹	THA⁵¹		2.62²⁵
	6⁹	–4.264²⁷
	5.40¹⁰	–4.08²⁹
	5.405¹¹	–4.234³⁴
	5.377¹²	–4.08³⁵
	5.424¹³	–4.30³⁷
		–4.15³⁹

Notes.

^(a)

Age estimates are based on: T_iso isochrone fitting, T_Li lithium abundance, T_gyro gyrochronology, T_HK Ca ii H&K emission, T_X X-ray emission.

^(b)

Labels for kinematic groups: “AB” AB Dor Moving Group, “HLA” Her-Lyr Association, “Hya” Hyades Supercluster, “IC” IC 2391 Supercluster, “LA” Local Association, “Ple” Pleiades Moving Group, “UMa” UMa Moving Group, “THA” Tuc-Hor Association, “TWA” TW Hya Association.

Reference.

⁽¹⁾

Hooten & Hall (1990);

⁽²⁾

Strassmeier & Rice (2006);

⁽³⁾

Messina et al. (2011);

⁽⁴⁾

Strassmeier et al. (2000);

⁽⁵⁾

Henry et al. (1995b);

⁽⁶⁾

Gaidos et al. (2000);

⁽⁷⁾

Kajatkari et al. (2015);

⁽⁸⁾

Petit et al. (2008);

⁽⁹⁾

Baliunas et al. (1996a);

⁽¹⁰⁾

Messina & Guinan (1996);

⁽¹¹⁾

Strassmeier et al. (1997);

⁽¹²⁾

Messina et al. (1999);

⁽¹³⁾

Messina & Guinan (2002);

⁽¹⁴⁾

Fekel et al. (1986a);

⁽¹⁵⁾

Strassmeier & Hall (1988);

⁽¹⁶⁾

Jetsu (1993);

⁽¹⁷⁾

Kővári et al. (2004);

⁽¹⁸⁾

Lehtinen et al. (2012);

⁽¹⁹⁾

Olspert et al. (2015);

⁽²⁰⁾

Lehtinen et al. (2011);

⁽²¹⁾

Strassmeier et al. (2003);

⁽²²⁾

Marsden et al. (2006);

⁽²³⁾

Järvinen et al. (2008);

⁽²⁴⁾

Huber et al. (2009);

⁽²⁵⁾

Biazzo et al. (2009);

⁽²⁶⁾

López-Santiago et al. (2010);

⁽²⁷⁾

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⁽²⁸⁾

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⁽²⁹⁾

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⁽³⁰⁾

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⁽³¹⁾

Jenkins et al. (2011);

⁽³²⁾

Noyes et al. (1984);

⁽³³⁾

Soderblom & Mayor (1993);

⁽³⁴⁾

Gray et al. (2006);

⁽³⁵⁾

Mishenina et al. (2012);

⁽³⁶⁾

Wright et al. (2004);

⁽³⁷⁾

White et al. (2007);

⁽³⁸⁾

Busà et al. (2007);

⁽³⁹⁾

Martínez-Arnáiz et al. (2010);

⁽⁴⁰⁾

Plavchan et al. (2009);

⁽⁴¹⁾

Montes et al. (2001a);

⁽⁴²⁾

Henry et al. (1996);

⁽⁴³⁾

Vidotto et al. (2014);

⁽⁴⁴⁾

Hempelmann et al. (1995);

⁽⁴⁵⁾

López-Santiago et al. (2003);

⁽⁴⁶⁾

Montes et al. (2001b);

⁽⁴⁷⁾

Frasca et al. (2010);

⁽⁴⁸⁾

Zuckerman & Song (2004);

⁽⁴⁹⁾

López-Santiago et al. (2006);

⁽⁵⁰⁾

McCarthy & White (2012);

⁽⁵¹⁾

Nakajima & Morino (2012);

⁽⁵²⁾

Fuhrmann (2004).

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