Velocities of M67 main-sequence and giant stars (Pasquini+, 2011)

Details Velocities of M67 main-sequence and giant stars (Pasquini+, 2011) Velocities of M67 main-sequence and giant stars (Pasquini+, 2011)

Jan 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011ycat..35269127p&link_type=abstract

VizieR On-line Data Catalog: J/A+A/526/A127. Originally published in: 2011A&A...526A.127P

Physics

Clusters: Open, Stars: Dwarfs, Stars: Giant, Radial Velocities, Rotational Velocities

Scientific paper

We observed 144 main-sequence stars and cool giants in the M67 open cluster using the ESO FEROS spectrograph and obtained radial velocities by means of cross-correlation with a spectral template. Binaries and doubtful members were not analyzed, and average spectra were created for different classes of stars.
(1 data file).

Affiliated with

Also associated with

No associations

Rating

Velocities of M67 main-sequence and giant stars (Pasquini+, 2011) 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 Velocities of M67 main-sequence and giant stars (Pasquini+, 2011), we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Velocities of M67 main-sequence and giant stars (Pasquini+, 2011) will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1549398