DSpace JSPUI
DSpace preserves and enables easy and open access to all types of digital content including text, images, moving images, mpegs and data sets
Learn More
Please use this identifier to cite or link to this item:
http://hdl.handle.net/2248/672| Title: | Spectrophotometry of Nova Coronae Austrinae, 1981 |
| Authors: | Shylaja, B. S |
| Keywords: | Novae Spectrum Analysis Stellar Spectrophotometry Black Body Radiation Electron Density (Concentration) Emission Spectra Hydrogen Ions Line Spectra Stellar Envelopes Ion Density (Concentration) |
| Issue Date: | Oct-1984 |
| Publisher: | D. Reidel Publishing Co. |
| Citation: | Astrophysics and Space Science, Vol. 104, No. 1, pp. 163 - 168 |
| Abstract: | Spectrophotometric observations of Nova Coronae Austrinae 1981, during its nebular phase are reported. The various emission lines are identified. The electron densities and the mass of the ionized hydrogen in the shell have been calculated. The excess flux in the red continuum probably indicates the appearance of the dust component. |
| URI: | http://hdl.handle.net/2248/672 |
| ISSN: | 0004-640X |
| Appears in Collections: | IIAP Publications |
Files in This Item:
| File | Description | Size | Format | |
|---|---|---|---|---|
| Spectrophotometry of Nova Coronae Austrinae | 370.64 kB | Adobe PDF |  View/Open |
Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.