J/MNRAS/403/2157ivo://CDS.VizieR/J/MNRAS/403/2157doi:10.26093/cds/vizier.74032157CDSHoudebine E.R.2024-07-11T20:16:12Z2010-11-26T14:44:01ZCDS support team

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

cds-question@unistra.frlate-type-starsmagnetic-fieldsspectroscopyWe report on high-resolution observations of two dM1 stars: Gl 867A, an active dM1e star, and Gl 205, a less active dM1 star. The wavelength coverage is from 3890 to 6820{AA} with a resolving power of about 45000. The difference spectrum of these two stars allows us to make a survey of spectral lines sensitive to magnetic activity.2010MNRAS.403.2157Hhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/403/2157CatalogResearchIsServedByTAP VizieR generic servicehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/403/2157https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/403/2157http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/403/2157https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/403/2157https://vizier.iucaa.in/viz-bin/votable?-source=J/MNRAS/403/2157http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/MNRAS/403/2157GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapOpticaldefaultJ/MNRAS/403/2157/table1aTotal results for each Flux setsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintdEW? Difference equivalent widths between Gl867A and Gl 2050.1pmspect.line.eqWidth;arith.diffintnullableFluxContinuum flux from Allard et al. (1997ARA&A..35..137A) (in 10^5^erg/cm2/s)hW.m**-2phot.fluxfloatlam.FFlux wavelength ({AA})0.1nmem.wlintprimarydFluxDifference radiative losses in the lines (1)10W.m**-2phot.fluxfloatNo? Order number of the corresponding spectral ordermeta.idintnullableJ/MNRAS/403/2157/table1List of the spectral lines sensitive to chromospheric activityrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintlambda0? Vacuum wavelength0.1nmem.wlfloatnullablelambda? Gl 205 wavelength0.1nmem.wlfloatnullabledEWDifference equivalent widths between Gl867A and Gl 2050.1pmspect.line.eqWidth;arith.diffintFluxContinuum flux from Allard et al. (1997ARA&A..35..137A) (in 10^5^erg/cm2/s)hW.m**-2phot.fluxfloatlam.FFlux wavelength0.1nmem.wlintdFluxDifference radiative losses in the lines10W.m**-2phot.fluxfloatIdentLine identificationmeta.id;spect.linecharNo? Order number of the corresponding spectral ordermeta.idintnullableRemOriginal catalog from which we identified each linemeta.notechar