The chemical composition of the Orion star forming region - I. Homogeneity of O and Si abundances in B-type stars

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Table 2:

Projected rotational velocities derived for the studied stars.
HD	v sin i^a	$\Theta_{\rm g}$ ^a	HD	v sin i	$\Theta_{\rm g}$
HD 36512	15	30	HD 37744	37	00
HD 37020	55	00	HD 36285	<10	20
HD 36960	23	40	HD 36629	<10	15
HD 37042	31	00	HD 35039	<12	15
HD 36591	08	19	HD 36430	<15	25
HD 36959	12	12	HD 35912	<12	20
HD 35299	<08	12

Notes. ^(a) Both quantities in km s^-1.

Source LaTeX | All tables | In the text

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