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Time Dependence of the UV Resonance Lines in the Cataclysmic Variable Star VW Hyi
| Content Provider | Scilit |
|---|---|
| Author | Özkan, M. T. Ak, T. Saygac, A. T. Esenoglu, H. H. Guler, S. |
| Copyright Year | 1995 |
| Description | In this work, we study orbital variations in the ultraviolet resonance lines of the SU UMa type dwarf nova VW Hyi examining spectra in the data archive of the International Ultraviolet Explorer (IUE). We show that VW Hyi exhibits an orbital and long term variability in terms of UV line profiles and continuum flux at 1450 Å during superoutburst. |
| Related Links | https://www.cambridge.org/core/services/aop-cambridge-core/content/view/24071FD6678D367FFD97E06743DFFF5E/S0252921100035193a.pdf/div-class-title-time-dependence-of-the-uv-resonance-lines-in-the-cataclysmic-variable-star-vw-hyi-a-href-fn01-ref-type-fn-a-div.pdf |
| Ending Page | 281 |
| Page Count | 2 |
| Starting Page | 280 |
| ISSN | 02529211 |
| DOI | 10.1017/s0252921100035193 |
| Journal | International Astronomical Union Colloquium |
| Volume Number | 151 |
| Language | English |
| Publisher | Cambridge University Press (CUP) |
| Publisher Date | 1995-01-01 |
| Access Restriction | Open |
| Subject Keyword | International Astronomical Union Colloquium Astronomy and Astrophysics |
| Content Type | Text |
| Resource Type | Article |