Doppler imaging combined with high-cadence photometry - I. Revisiting the surface of a pre-main-sequence flare star PW Andromedae

Open Access

Table 2

Adopted stellar parameters.

Parameter	Value
v sin i(km s⁻¹)	$21 . 9_{- 1.9}^{+ 2.8}^{a}$ $Mathematical equation: $21.9_{-1.9}^{+2.8}{ }^{\mathrm{a}}$$
P_rot (days)	1.756604 ± 0.000015^b
T₀ (HJD)	2453200.0^c
M(M_⊙)	0.85 ± 0.05^d
R(R_⊙)	$1 . 16_{- 0.11}^{+ 0.15}^{c}$ $Mathematical equation: $1.16_{-0.11}^{+0.15}{ }^{\mathrm{c}}$$
i(^°)	46.0 ± 7^c
T_eff(K)	5080 ± 28^b
T_spot(K)	3800^c
log g	4.40 ± 0.09^b
[Fe/H]	−0.14 ± 0.02^b
Microturbulence (km s⁻¹)	1.93 ± 0.09^b
Macroturbulence (km s⁻¹)	3.25 ± 0.06^b

Notes. ^(a) This study. ^(b) Bahar et al. (2024). ^(c) Strassmeier & Rice (2006). ^(d) Folsom et al. (2016).

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.