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dc.contributor.authorLopez-Santiago, J.
dc.contributor.authorMontes, D.
dc.contributor.authorGalvez-Ortiz, M.C.
dc.contributor.authorCrespo-Chacon, I.
dc.contributor.authorMartinez-Arnaiz, R.M.
dc.contributor.authorFernandez-Figueroa, M.J.
dc.contributor.authorDe Castro, E.
dc.contributor.authorCornide, M.
dc.date.accessioned2010-07-06T09:33:31Z
dc.date.available2010-07-06T09:33:31Z
dc.date.issued2010
dc.identifier.citationLopez-Santiago , J , Montes , D , Galvez-Ortiz , M C , Crespo-Chacon , I , Martinez-Arnaiz , R M , Fernandez-Figueroa , M J , De Castro , E & Cornide , M 2010 , ' A high-resolution spectroscopic survey of late-type stars: chromospheric activity, rotation, kinematics, and age ' , Astronomy and Astrophysics , vol. 514 . https://doi.org/10.1051/0004-6361/200913437
dc.identifier.issn0004-6361
dc.identifier.otherPURE: 154700
dc.identifier.otherPURE UUID: f7686a84-315d-49eb-af39-0ccfdeb99667
dc.identifier.otherdspace: 2299/4627
dc.identifier.otherScopus: 77952927118
dc.identifier.urihttp://hdl.handle.net/2299/4627
dc.descriptionOriginal article can be found at: http://www.aanda.org/ Copyright The European Southern Observatory (ESO) DOI: 10.1051/0004-6361/200913437
dc.description.abstractAims. 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.en
dc.language.isoeng
dc.relation.ispartofAstronomy and Astrophysics
dc.rightsOpen
dc.titleA high-resolution spectroscopic survey of late-type stars: chromospheric activity, rotation, kinematics, and ageen
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.description.statusPeer reviewed
dc.relation.schoolSchool of Physics, Astronomy and Mathematics
dcterms.dateAccepted2010
rioxxterms.versionofrecordhttps://doi.org/10.1051/0004-6361/200913437
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue
herts.rights.accesstypeOpen


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