Radial velocity for the open cluster NGC 2420

Details Radial velocity for the open cluster NGC 2420 Radial velocity for the open cluster NGC 2420

Oct 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987pasp...99.1076l&link_type=abstract

Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 99, Oct. 1987, p. 1076-1079.

Astronomy and Astrophysics

Astronomy

12

Giant Stars, Open Clusters, Radial Velocity, Stellar Spectra, Charge Coupled Devices, Error Analysis

Scientific paper

The authors present radial velocities for the bright stars, nine of them giants, in the old open cluster NGC 2420 from high-resolution spectra obtained with the 2.1-meter coudé spectrograph at KPNO. The mean cluster velocity is found to be 70.0±1.4 (rms) km s-1 based on these velocity measurements. Among the ten stars observed, two have been confirmed to be nonmembers from their radial-velocity data. In addition, two barium stars in the sample have shown variable velocities when compared with previous observations.

Affiliated with

Also associated with

No associations

Rating

Radial velocity for the open cluster NGC 2420 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 for the open cluster NGC 2420, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Radial velocity for the open cluster NGC 2420 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1776598