J/A+A/487/293ivo://CDS.VizieR/J/A+A/487/293doi:10.26093/cds/vizier.34870293CDSFuhrmeister B.Liefke C.Schmitt J.H.M.M.Reiners A.2008-09-21T08:49:06Z2008-09-21T08:44:23ZCDS support team

CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France

cds-question@unistra.frlate-type-starsm-starsFlares on dM stars contain plasmas at very different temperatures and thus affect a wide wavelength range in the electromagnetic spectrum. While the coronal properties of flares are studied best in X-rays, the chromosphere of the star is observed best in the optical and ultraviolet ranges. Therefore, multiwavelength observations are essential to study flare properties throughout the atmosphere of a star.2008A&A...487..293Fhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/487/293CatalogResearchIsServedByTAP VizieR generic servicerelated-toJ/A+A/439/1137 : PHOENIX model chromospheres of M dwarfs (Fuhrmeister+, 2005)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/487/293https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/487/293http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/487/293https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/487/293https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/487/293http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/487/293GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapOpticaldefaultJ/A+A/487/293/table1Catalog of chromospheric emission linesIonIon codemeta.code;phys.atmol.ionStagecharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintlambda1? Measured wavelength0.1nmem.wldoublenullableFWHM? Line FWHM0.1nmspect.line.width;spect.linefloatnullableFlux? Line fluxmW.m**-2phot.fluxdoublenullablelambda2? Cataloged wavelength0.1nmem.wldoublenullableMult? Multiplet numbermeta.id;meta.mainintnullableIDflagIdentification status flag (1)meta.codeintRemRemarks (2)meta.notechar