Rotation velocities of dwarf M stars (Houdebine, 2010)

Details Rotation velocities of dwarf M stars (Houdebine, 2010) Rotation velocities of dwarf M stars (Houdebine, 2010)

Feb 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011ycat..74071657h&link_type=abstract

VizieR On-line Data Catalog: J/MNRAS/407/1657. Originally published in: 2010MNRAS.407.1657H

Physics

Stars: Dwarfs, Rotational Velocities

Scientific paper

We have measured vsini for a selected sample of dM1-type stars. We give 114 measurements of vsini for 88 different stars, and six upper detection limits. These are the first measurements of vsini for most of the stars studied here. This represents the largest sample of vsini measurements for M dwarfs at a given spectral type. For these measurements, we used four different spectrographs: HARPS (ESO), SOPHIE (OHP), ELODIE (OHP) and UVES (ESO). Two of these spectrographs (HARPS and SOPHIE) are particularly stable in wavelength since they were designed for exoplanet searches.
(2 data files).

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