A catalog of rotational and radial velocitiesfor evolved stars

Aims.The present paper describes the first results of an observational program intended to refine and extend the existing $v \sin i$ measurements of metal-poor stars, with an emphasis on field evolved stars. Methods.The survey was carried out with the FEROS and CORALIE spectrometers. For the $v \sin...

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Published inAstronomy and astrophysics (Berlin) Vol. 458; no. 3; pp. 895 - 898
Main Authors De Medeiros, J. R., Silva, J. R. P., do Nascimento Jr, J. D., Canto Martins, B. L., da Silva, L., Melo, C., Burnet, M.
Format Journal Article
LanguageEnglish
Published EDP Sciences 01.11.2006
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Summary:Aims.The present paper describes the first results of an observational program intended to refine and extend the existing $v \sin i$ measurements of metal-poor stars, with an emphasis on field evolved stars. Methods.The survey was carried out with the FEROS and CORALIE spectrometers. For the $v \sin i$ measurements, obtained from spectral synthesis, we estimate an uncertainty of about 2.0 ${\rm km\,s}^{-1}$. Results.Precise rotational velocities ${v\sin i}$ are presented for a large sample of 100 metal-poor stars, most of them evolving off the main–sequence. For the large majority of the stars composing the present sample, rotational velocities have been measured for the first time.
Bibliography:istex:C02B63B685EED1A621E2FEA7EF291BCE9809A970
other:2006A%26A...458..895D
publisher-ID:aa5642-06
ark:/67375/80W-PXTQ1Z36-S
ISSN:0004-6361
1432-0746
DOI:10.1051/0004-6361:20065642