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Iue observations of the 1987 superoutburst of the dwarf nova z cha
| Content Provider | NASA Technical Reports Server (NTRS) |
|---|---|
| Author | Naylor, T. Harlaftis, E. Hassall, B. J. M. Sonneborn, G. Charles, P. A. |
| Copyright Year | 1988 |
| Description | Low resolution IUE observations of the dwarf nova Z Cha during superoutburst are presented. These cover most of the development of the outburst and have sufficient time resolution to probe continuum and line behavior on orbital phase. The observed modulation on this phase is very similar to that observed in the related object OY Car. The results imply the presence of a cool spot on the edge of the edge of the accretion disk, which periodically occults the brighter inner disk. Details of the line behavior suggest that the line originated in an extended wind-emitting region. In contrast to archive spectra obtained in normal outburst, the continuum is fainter and redder, indicating that the entire superoutburst disk may be geometrically thicker than during a normal outburst. |
| File Size | 236676 |
| Page Count | 4 |
| File Format | |
| Alternate Webpage(s) | http://archive.org/details/NASA_NTRS_Archive_19890001344 |
| Archival Resource Key | ark:/13960/t88h3hm40 |
| Language | English |
| Publisher Date | 1988-06-01 |
| Access Restriction | Open |
| Subject Keyword | Astronomy Bursts Spaceborne Astronomy Ultraviolet Spectra Iue Dwarf Novae Periodic Variations Ultraviolet Astronomy Ntrs Nasa Technical Reports ServerĀ (ntrs) Nasa Technical Reports Server Aerodynamics Aircraft Aerospace Engineering Aerospace Aeronautic Space Science |
| Content Type | Text |
| Resource Type | Article |