Abundance analysis of prime B-type targets for asteroseismology - II. B6–B9.5 stars in the field of view of the CoRoT satellite | A&A

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Table A.1:

Stellar parameters and rotational velocites of the test synthetic spectra.
$T_{\rm eff}$	$\log g$	$\xi$	$V\sin i$
[K]		[km s^-1]	[km s^-1]
10 000	4.0	2	10, 50, 100, 150, 200
12 000	4.0	2	10, 50, 100, 150, 200
14 000	4.0	2	10, 50, 100, 150, 200

Source LaTeX | All tables | In the text