EDP Sciences logo
Subscriber Authentication Point
Search
Menu
Home All issues Volume 501 / No 1 (July I 2009) A&A, 501 1 (2009) 291-295 Full HTML
Free Access
   

Table 3:

Orbital solutions deduced from different lines (Col. 1).
Line P e $\omega$ K1 $\gamma_1$ rms
  (d)   ($^\circ$) (km s-1) (km s-1) (km s-1)
H$\beta $ 4.24021 0.058 $\pm $ 0.006 140 $\pm $ 5 117.0 $\pm $ 0.5 $-29.6 \pm$ 0.6 4.9
He  II \l4686 4.24029 0.085 $\pm $ 0.003 153 $\pm $ 1 124.4 $\pm $ 0.2 $-17.3 \pm$ 0.3 2.0
He  I \l4922 4.24023 0.057 $\pm $ 0.006 148 $\pm $ 4 107.7 $\pm $ 0.4 $-17.9 \pm$ 0.5 3.8
He  I \l5015 4.24015 0.059 $\pm $ 0.006 150 $\pm $ 4 112.1 $\pm $ 0.4 $-22.2 \pm$ 0.6 4.0
He  I \l5876 4.24021 0.069 $\pm $ 0.004 151 $\pm $ 2 115.9 $\pm $ 0.3 $-22.4 \pm$ 0.4 2.9
He  I \l6678 4.24022 0.061 $\pm $ 0.005 151 $\pm $ 3 114.4 $\pm $ 0.4 $-14.7 \pm$ 0.5 3.2

The usual notations for the orbital elements have been used. Quoted uncertainties are the 1-$\sigma $ error bars.


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.