Rotational velocities of A-type stars - II. Measurement of in the northern hemisphere (original) (raw)

A&A 393, 897-911 (2002)

II. Measurement of ${v\sin i}$ in the northern hemisphere

1 Observatoire de Genève, 51 chemin des Maillettes, 1290 Sauverny, Switzerland
2 GEPI/CNRS FRE 2459, Observatoire de Paris, 5 place Janssen, 92195 Meudon Cedex, France
3 CNRS, Institut d'Astrophysique de Paris, 98bis boulevard Arago, 75014 Paris, France

Corresponding author: F. Royer, frederic.royer@obs.unige.ch

Received: 25 February 2002
Accepted: 19 June 2002

Abstract

This work is the second part of the set of measurements of${v\sin i}$ for A-type stars, begun by Royer et al. ([CITE]). Spectra of 249 B8 to F2-type stars brighter than $V=7$ have been collected at Observatoire de Haute-Provence (OHP). Fourier transforms of several line profiles in the range 4200–4600 Å are used to derive ${v\sin i}$ from the frequency of the first zero. Statistical analysis of the sample indicates that measurement error mainly depends on ${v\sin i}$ and this relative error of the rotational velocity is found to be about 5% on average. The systematic shift with respect to standard values from Slettebak et al. ([CITE]), previously found in the first paper, is here confirmed. Comparisons with data from the literature agree with our findings: ${v\sin i}$ values from Slettebak et al. are underestimated and the relation between both scales follows a linear law ${v\sin i}_{\rm new} = 1.03\,{v\sin i}_{\rm old}+7.7$. Finally, these data are combined with those from the previous paper (Royer et al. [CITE]), together with the catalogue of Abt & Morrell ([CITE]). The resulting sample includes some 2150 stars with homogenized rotational velocities.

Key words: techniques: spectroscopic / stars: early-type / stars: rotation


*

Based on observations made at Observatoire de Haute Provence (CNRS), France.

**

Tables [see full text] and [see full text] are only available in electronic form at the CDS via anonymous ftp to cdsarc.u-strasbg.fr (130.79.125.5) or via http://cdsweb.u-strasbg.fr/cgi-bin/qcat?J/A+A/393/897

© ESO, 2002

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