Abstract
Rotational and radial velocities have been measured for 1589 evolved stars of spectral types F, G, and K and luminosity classes IV, III, II, and Ib, based on observations carried out with the CORAVEL spectrometers. The precision in radial velocity is better than 0.30 km s -1 per observation, whereas rotational velocity uncertainties are typically 1.0 km s -1 for subgiants and giants and 2.0 km s -1 for class II giants and Ib supergiants.
Originalsprog | Engelsk |
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Artikelnummer | A126 |
Tidsskrift | Astronomy & Astrophysics |
Vol/bind | 561 |
ISSN | 0004-6361 |
DOI | |
Status | Udgivet - 1 jan. 2014 |