V1974 Cyg IUE spectroscopy Virtual Observatory Resource

Authors

1. Cassatella A.
2. Lamers H.J.G.L.M.
3. Rossi C.
4. Altamore A.,Gonzalez-Riestra R.

Published by

CDS

Abstract

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.

Keywords

1. variable-stars
2. cataclysmic-variable-stars
3. radial-velocity
4. spectroscopy
5. ultraviolet-astronomy

Bibliographic source Bibcode

2004A&A...420..571C

See also HTML

https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/420/571

IVOA Identifier IVOID

ivo://CDS.VizieR/J/A+A/420/571

Document Object Identifer DOI

doi:10.26093/cds/vizier.34200571

Access

Web browser access HTML

http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/420/571
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/420/571
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/420/571

IVOA Table Access TAP

http://tapvizier.cds.unistra.fr/TAPVizieR/tap
Run SQL-like queries with TAP-enabled clients (e.g., TOPCAT).