J/A+A/385/986ivo://CDS.VizieR/J/A+A/385/986doi:10.26093/cds/vizier.33850986CDSFremat Y.Zorec J.Hubert A.-M.Cidale L.S.Rohrmann R.D.,Desert J.-M.Ferlet R.Vidal-Madjar A.2002-05-12T06:46:34Z2002-05-12T06:46:30ZCDS support team

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

cds-question@unistra.frNew spectra have been obtained for the pole-on Be star HR 5223 (HD 120991) using the Far Ultraviolet Satellite Explorer (FUSE). We give a complete description of the far-UV spectral range (920 to 1180{AA}). The spectra are affected by strong blends with interstellar lines and molecular bands that also significantly lower the energy distribution of the star. We produce a synthetic spectrum of the interstellar medium (ISM) to determine the column densities of several elements (H_2_, H I, N I, O I ...) seen towards HR 5223 and to disentangle the components due to the ISM, the photosphere and/or to the circumstellar envelope.2002A&A...385..986Fhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/385/986CatalogResearchIsServedByTAP VizieR generic servicehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/385/986https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/385/986http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/385/986https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/385/986https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/385/986http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/385/986GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapFUSEOpticaldefaultJ/A+A/385/986/table2Photospheric and interstellar line identification listrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintWobsObserved wavelength0.1nmem.wlfloatWthTheoretical wavelength0.1nmem.wlfloatIdLine identificationmeta.idcharn_Id[*] *: photospheric linemeta.notechar