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

S. Simón-Díaz

doi:10.1051/0004-6361/200913120

Home

All issues

Volume 510 (February 2010)

A&A, 510 (2010) A22

Full HTML

Free Access

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

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.