Free Access
 

 

Table 2:

Main sequence A-type stars in which evidence of velocity fields is directly detected in line profiles.
HD other spectral binarity \ensuremath {T_{{\rm e}}} $\xi $ depressed line shape \ensuremath{v_{\rm e} \sin i}
    type       blue wing discrepancy weak lines strong lines
        (K) ( \ensuremath{{\rm km~s}^{-1}})     ( \ensuremath{{\rm km~s}^{-1}}) ( \ensuremath{{\rm km~s}^{-1}})
2421 A HR 104 A A2Vs SB2 10 000 1.0 weak none 3.5 3.5
72660 HR 3383 A1V   9650 2.3 weak weak 5.0 6.1
114330 $\theta $ Vir A1Vs VB2 9250 1.3 weak weak 4.0 5.5
157486 A HR 6470 A A0V SB2 9150 1.9 weak weak 1.5 3.5
27962 68 Tau A2IV m SB1 8975 2.0 weak weak 11 11.5
103578 A 95 Leo A A3V SB2 8300 2.0 strong strong 3 9
107168 8 Com A8 m   8150 3.0 weak weak 13 14
108642 A HR 4750 A A2 m SB1 8100 4.0 strong strong 2 10
209625 32 Aqr A5 m SB1 7700 4.0 strong strong 4.5 10

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.