V1974 Cyg IUE spectroscopy

DOI

We have carried out a detailed analysis of the IUE archival high resolution spectra of the classical nova V1974 Cyg 1992. The main UV resonance lines show P Cygni profiles in the first days, which change into symmetric pure emission lines, and then slowly become fainter and narrower. Lines of higher ionization species reach their peak luminosity later than those of low ionization.

Identifier
DOI http://doi.org/10.26093/cds/vizier.34200571
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/A+A/420/571
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/420/571
Related Identifier https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/420/571
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/A+A/420/571
Provenance
Creator Cassatella A.; Lamers H.J.G.L.M.; Rossi C.; Altamore A.,Gonzalez-Riestra R.
Publisher CDS
Publication Year 2004
Rights https://cds.unistra.fr/vizier-org/licences_vizier.html
OpenAccess true
Contact CDS support team <cds-question(at)unistra.fr>
Representation
Resource Type Dataset; AstroObjects
Discipline Astrophysics and Astronomy; Exoplanet Astronomy; Interdisciplinary Astronomy; Natural Sciences; Observational Astronomy; Physics; Stellar Astronomy