Zeeman-Doppler imaging of five young solar-type stars

Free Access

Table 3.

Stellar parameters and parameters used in the ZDI inversion.

Parameter	BE Cet	χ¹ Ori	HD 29615	HD 35296	V1358 Ori
P_rot [d]	7.676 ^(a)	5.022 ^(a)	2.32 ^(b)	3.493 ^(a)	1.3571 ^(c)
τ_conv [d]	12.51	8.76	9.72	6.12	8.37
Ro	0.61	0.57	0.24	0.57	0.16
v sin i [km s⁻¹]	7.0 ^(d)	9.8 ^(d)	18.5 ^(e)	15.9 ^(f)	41.3 ^(e)
Inclination [°]	65 ^(g)	65 ^(g)	62 ^(e)	65 ^(f)	59 ^(e)
R (from Eq. (4)) [R_⊙]	1.17	1.07	0.96	1.21	1.29
R (literature) [R_⊙]	1.00 ^(h)	1.05 ^(h)	0.96 ^(b)	1.10 ^(f)	1.05 ⁽ⁱ⁾/1.08 ^(j)
T_eff [K]	5837 ^(d)	5882 ^(d)	5820 ^(f)	6170 ^(k)	6032 ^(l)
Effective Landé g factor	1.216	1.217	1.213	1.218	1.218

References.

^(a)

Lehtinen et al. (2020),

^(b)

Vidotto et al. (2014),

^(c)

Kriskovics et al. (2019),

^(d)

Valenti & Fischer (2005),

^(e)

Hackman et al. (2016),

^(f)

Waite et al. (2015),

^(g)

Rosén et al. (2016),

^(h)

Takeda et al. (2007),

⁽ⁱ⁾

Vican & Schneider (2014),

^(j)

Zuckerman et al. (2011),

^(k)

Casagrande et al. (2011),

^(l)

McDonald et al. (2012).

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.