University of Hertfordshire

From the same journal

From the same journal


  • J. Lopez-Santiago
  • D. Montes
  • M.C. Galvez-Ortiz
  • I. Crespo-Chacon
  • R.M. Martinez-Arnaiz
  • M.J. Fernandez-Figueroa
  • E. De Castro
  • M. Cornide
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Original languageEnglish
JournalAstronomy and Astrophysics
Publication statusPublished - 2010


Aims. We present a compilation of spectroscopic data from a survey of 144 chromospherically active young stars in the solar neighborhood, which may be used to investigate different aspects of its formation and evolution in terms of kinematics and stellar formation history. The data have already been used by us in several studies. With this paper, we make all these data accessible to the scientific community for future studies on different topics. Methods. We performed spectroscopic observations with echelle spectrographs to cover the entirety of the optical spectral range simultaneously. Standard data reduction was performed with the IRAF echelle package. We applied the spectral subtraction technique to reveal chromospheric emission in the stars of the sample. The equivalent width of chromospheric emission lines was measured in the subtracted spectra and then converted to fluxes using equivalent width-flux relationships. Radial and rotational velocities were determined by the cross-correlation technique. Kinematics, equivalent widths of the lithium line λ6707.8 Å and spectral types were also determined.


Original article can be found at: Copyright The European Southern Observatory (ESO) DOI: 10.1051/0004-6361/200913437

ID: 154700