Open Access

Table 3.

Top: Most probable parameters of Rasalhague with 2D-ESTER models using the interferometric constraint on equatorial radius by Monnier et al. (2010). Bottom: 2D-ESTER concordance model of Rasalhague that fits all the observed quantities. The M10 column shows values derived by Monnier et al. (2010).

Stellar parameter Our derivation
i (°) 68.9 ± 5.6
M (M) 2.225 ± 0.021
Lapp (L) 27.08 ± 0.87
Req (R) 2.858 ± 0.009
Ωeqc 0.628 ± 0.026
Xcore/Xenv 0.361 ± 0.016
TIRFM (K) 8035 ± 63
c1 1.310 ± 0.163
c2 4.748 ± 0.137

Best Rasalhague model
Parameters This work M10

M (M) 2.225 2.18 ± 0.02
L (L) 29.3 31.3 ± 1
Rpole (R) 2.383 2.388 ± 0.013
Req (R) 2.859 2.858 ± 0.015
ϵ = 1 − Rpole/Req 0.167 0.164
Teffpole (K) 9051 9384 ± 154
Teffeq (K) 7609 7569 ± 124
Veq (km/s) 242
Protpole (h) 14.76
Proteq(h) 14.33 14.55 ± 0.35
Xenv 0.72
Xcore 0.260
Z 0.019
i(°) 69
Lapp (L) 26.9 25.6

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.