Radial velocity measurements of B stars in the Scorpius-Centaurus association

Details Radial velocity measurements of B stars in the Scorpius-Centaurus association Radial velocity measurements of B stars in the Scorpius-Centaurus association

2006-01-27

arxiv.org/abs/astro-ph/0601643v1

Astronomy and Astrophysics

Astrophysics

accepted for publication in A&A

Scientific paper

10.1051/0004-6361:20041614

We derive single-epoch radial velocities for a sample of 56 B-type stars members of the subgroups Upper Scorpius, Upper Centaurus Lupus and Lower Centaurus Crux of the nearby Sco-Cen OB association. The radial velocity measurements were obtained by means of high-resolution echelle spectra via analysis of individual lines. The internal accuracy obtained in the measurements is estimated to be typically 2-3 km/s, but depends on the projected rotational velocity of the target. Radial velocity measurements taken for 2-3 epochs for the targets HD120307, HD142990 and HD139365 are variable and confirm that they are spectroscopic binaries, as previously identified in the literature. Spectral lines from two stellar components are resolved in the observed spectra of target stars HD133242, HD133955 and HD143018, identifying them as spectroscopic binaries.

Affiliated with

Also associated with

No associations

Rating

Radial velocity measurements of B stars in the Scorpius-Centaurus association does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Radial velocity measurements of B stars in the Scorpius-Centaurus association, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Radial velocity measurements of B stars in the Scorpius-Centaurus association will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-505896