Radial velocities, rotations, and duplicity of a sample of early F-type dwarfs

Astronomy and Astrophysics – Astronomy

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Methods: Statistical, Techniques: Radial Velocities, Stars: Binaries: Spectroscopic, Stars: Kinematics, Galaxy: Solar Neighbourhood

Scientific paper

We present new radial and rotational velocities for 595 nearby early F dwarfs, based on digital spectra cross-correlated with individually optimised synthetic template spectra. The selection of optimum templates, the determination of rotational velocities, and the extraction of velocities from the blended spectra of double-lined spectroscopic binaries are discussed in some detail. We find 170 spectroscopic binaries in the sample and determine orbits for 18 double-lined and 2 single-lined binaries, including some spectroscopic triples. 73 stars are listed with too rapid rotation to yield useful radial velocities (i.e. v sin i > 120 km~s^-1). We discuss the binary frequency in the sample, and the influence of unrecognised binaries on the definition of clean metallicity groups of young F dwarfs and the determination of their kinematical properties. Tables 1, 5 and 6 are only available, and Tables 2-4 also available in electronic form at the CDS via anonymous ftp to cdsarc.u-strasbg.fr (130.79.128.5) or via http://cdsweb.u-strasbg.fr/Abstract.html.

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