525 datasets found

Keywords: dwarf stars

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  • NIR spectral of M-T dwarfs

    We present complete near-infrared (0.85-2.45um), low-resolution (R~100) spectra of a sample of 54 disk M-, L-, and T-dwarfs with reliable optical or near infrared spectral-type...
  • M dwarfs radial velocities

    We present radial velocity (RV) measurements of our sample of 40 M dwarfs from our planet search programme with VLT+UVES begun in 2000. Although with our RV precision down to...
  • Lithium in globular NGC 6397

    Most globular clusters are believed to host a single stellar population. They can thus be considered a good place to study the Spite plateau and to search for possible...
  • CoRoT-7 radial velocities

    We report on an intensive observational campaign carried out with HARPS at the 3.6m telescope at La Silla on the star CoRoT-7. Additional simultaneous photometric measurements...
  • Abundances in solar analogs

    We derive the abundance of 19 elements in a sample of 64 stars with fundamental parameters very similar to solar, which minimizes the impact of systematic errors in our...
  • Velocities of 43 nearby L dwarfs

    We present radial velocity measurements of a sample of L0-L8 dwarfs observed with VLT/UVES and Keck/HIRES. We combine these measurements with distance and proper motion from the...
  • Teff and Fbol from Infrared Flux Method

    Various effective temperature scales have been proposed over the years. Despite much work and the high internal precision usually achieved, systematic differences of order 100K...
  • Post common envelope binaries from SDSS. VIII

    We present the results of a large survey of post common envelope binaries (PCEBs) among white dwarf/main sequence (WDMS) binaries from the SDSS that allows to determine the...
  • Abundances of dwarfs and giants in 2 open clusters

    It has been suggested that the classical chemical analysis may be affected by systematic errors that would introduce abundance differences between dwarfs and giants. For some...
  • Lithium content of {omega} Cen

    A discrepancy has emerged between the cosmic lithium abundance inferred by the WMAP satellite measurement coupled with the prediction of the standard big-bang nucleosynthesis...
  • i'z' photometry of L5 and later dwarf candidates

    Thanks to recent and ongoing large scale surveys, hundreds of brown dwarfs have been discovered in the last decade. The Canada-France Brown Dwarf Survey is a wide-field survey...
  • HARPS XXIII: RV data for the 8 targets

    In this paper, we present our HARPS radial-velocity data for eight low-activity solar-type stars belonging to the HARPS volume-limited sample: HD6718, HD8535, HD28254, HD290327,...
  • A Jupiter-mass companion around HD 109246

    We report the detection of a Jupiter-mass planet discovered with the SOPHIE spectrograph mounted on the 1.93-m telescope at the Haute-Provence Observatory. The new planet orbits...
  • CN and CH line strengths in 12 globulars

    Globular clusters show star-to-star abundance variations for light elements that are not yet well understood. The preferred explanation involves a self-enrichment scenario,...
  • Velocities of M67 main-sequence and giant stars

    Precise analyses of stellar radial velocities is able to reveal intrinsic causes of the wavelength shifts of spectral lines (other than Doppler shifts due to radial motion),...
  • Rotating massive MS stars evolutionary models

    We present a dense grid of evolutionary tracks and isochrones of rotating massive main-sequence stars. We provide three grids with different initial compositions tailored to...
  • Physical parameters of PMS in open clusters

    Our aims are twofold: To determine the physical parameters of PMS members in young open clusters (YOCs), and to check and compare the performances of different model isochrones....
  • Activity indices and velocities for 890 stars

    In this work we present chromospheric activity indices, kinematics, radial-velocities, and rotational velocities for more than 850 FGK-type dwarfs and subgiant stars in the...
  • SDSS WD main-sequence binaries. XII.

    The complexity of the common-envelope phase and of magnetic stellar wind braking currently limits our understanding of close binary evolution. Because of their intrinsically...
  • Li and Na in globular cluster M4

    The abundance inhomogeneities of light elements observed in globular clusters (GCs), and notably the ubiquitous Na-O anti-correlation, are generally interpreted as evidence that...
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