EDP Sciences logo
Subscriber Authentication Point
Search
Menu
Home All issues Volume 506 / No 1 (October IV 2009) A&A, 506 1 (2009) 15-32 Full HTML
   

Table 9:

Global parameter posterior estimates for HD 49933. i represents the inclination angle of the star. $\nu _{\rm s}$ is the rotational splitting, Vl=1 and Vl=2 the relative height of l=1 and l=2 modes, respectively. $\Delta \nu $ represent the large separation.

Model		 $M^1_{\rm A}$ $M^1_{\rm B}$

Probability		 62.8% 0.2%
i $(^\circ$) median 52 23
$1 \sigma_+/1 \sigma_- $ $8\hspace{0.5mm}/\hspace{0.5mm}8$ $17\hspace{0.5mm}/\hspace{0.5mm}15$
  $2 \sigma_+$/ $2 \sigma_-$ $20\hspace{0.5mm}/\hspace{0.5mm}18$ $36\hspace{0.5mm}/\hspace{0.5mm}22$
$\nu _{\rm s}$ ( $\mu {\rm Hz}$) median 3.20 3.34
$1 \sigma_+/1 \sigma_- $ $0.28\hspace{0.5mm}/\hspace{0.5mm}0.26$ $0.34\hspace{0.5mm}/\hspace{0.5mm}0.35$
  $2 \sigma_+/2 \sigma_- $ $0.59\hspace{0.5mm}/\hspace{0.5mm}0.54$ $0.69\hspace{0.5mm}/\hspace{0.5mm}0.69$
Vl=1 median 1.00 0.93
$1 \sigma_+/1 \sigma_- $ $0.09\hspace{0.5mm}/\hspace{0.5mm}0.09$ $0.08\hspace{0.5mm}/\hspace{0.5mm}0.09$
  $2 \sigma_+/ 2 \sigma$ $0.20\hspace{0.5mm}/\hspace{0.5mm}0.17$ $0.19\hspace{0.5mm}/\hspace{0.5mm}0.15$
$\Delta \nu $ ( $\mu {\rm Hz}$) median 86.04 86.04
$1 \sigma_+/1 \sigma_- $ $0.13\hspace{0.5mm}/\hspace{0.5mm}0.14$ $0.14\hspace{0.5mm}/\hspace{0.5mm}0.16$
  $2 \sigma_+/2 \sigma_- $ $0.28\hspace{0.5mm}/\hspace{0.5mm}0.33$ $0.28\hspace{0.5mm}/\hspace{0.5mm}0.33$

Model		 $M^2_{\rm A}$ $M^2_{\rm B}$

Probability		 14% 23%
i $(^\circ$) median 50 28
$1 \sigma_+/1 \sigma_- $ $8\hspace{0.5mm}/\hspace{0.5mm}7$ $19\hspace{0.5mm}/\hspace{0.5mm}17$
  $2 \sigma_+$/ $2 \sigma_-$ $15\hspace{0.5mm}/\hspace{0.5mm}21$ $39\hspace{0.5mm}/\hspace{0.5mm}27$
$\nu _{\rm s}$ ( $\mu {\rm Hz}$) median 3.17 3.37
$1 \sigma_+/1 \sigma_- $ $0.27\hspace{0.5mm}/\hspace{0.5mm}0.25$ $0.32\hspace{0.5mm}/\hspace{0.5mm}0.35$
  $2 \sigma_+/2 \sigma_- $ $0.57\hspace{0.5mm}/\hspace{0.5mm}0.52$ $0.68\hspace{0.5mm}/\hspace{0.5mm}0.70$
Vl=1 median 1.11 1.22
$1 \sigma_+/1 \sigma_- $ $0.16\hspace{0.5mm}/\hspace{0.5mm}0.11$ $0.22\hspace{0.5mm}/\hspace{0.5mm}0.16$
  $2 \sigma_+/ 2 \sigma$ $0.36\hspace{0.5mm}/\hspace{0.5mm}0.21$ $0.52\hspace{0.5mm}/\hspace{0.5mm}0.28$
Vl=2 median 0.13 0.35
$1 \sigma_+/1 \sigma_- $ $0.14\hspace{0.5mm}/\hspace{0.5mm}0.09$ $0.21\hspace{0.5mm}/\hspace{0.5mm}0.15$
  $2 \sigma_+/2 \sigma_- $ $0.34\hspace{0.5mm}/\hspace{0.5mm}0.13$ $0.50\hspace{0.5mm}/\hspace{0.5mm}0.27$
$\Delta \nu $ ( $\mu {\rm Hz}$) median 86.05 86.00
$1 \sigma_+/1 \sigma_- $ $0.13\hspace{0.5mm}/\hspace{0.5mm}0.15$ $0.16\hspace{0.5mm}/\hspace{0.5mm}0.19$
  $2 \sigma_+/2 \sigma_- $ $0.30\hspace{0.5mm}/\hspace{0.5mm}0.42$ $0.32\hspace{0.5mm}/\hspace{0.5mm}0.42$
i represents the inclination angle of the star. $\nu _{\rm s}$ is the rotational splitting, Vl=1 and Vl=2 the relative height of l=1 and l=2 modes, respectively. $\Delta \nu $ represent the large separation.

Source LaTeX | All tables | In the text

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.