A copy of this work was available on the public web and has been preserved in the Wayback Machine. The capture dates from 2018; you can also visit the original URL.
The file type is
As a first step to study the influence that rotation has in the evolution of the most massive stars, we obtained the projected rotational velocity (vsini) of a sample of OB stars from clusters and associations. We found that most of our stars presentvsinilower than 200 km/s.doi:10.1017/s0074180900195154 fatcat:oxer6hsy5zdvzgem22rx4ktmhu