dc.contributor.author |
Shylaja, B. S |
|
dc.date.accessioned |
2006-01-05T04:10:46Z |
|
dc.date.available |
2006-01-05T04:10:46Z |
|
dc.date.issued |
1984-10 |
|
dc.identifier.citation |
Astrophysics and Space Science, Vol. 104, No. 1, pp. 163 - 168 |
en |
dc.identifier.issn |
0004-640X |
|
dc.identifier.uri |
http://hdl.handle.net/2248/672 |
|
dc.description.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. |
en |
dc.format.extent |
898771 bytes |
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dc.format.mimetype |
application/pdf |
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dc.language.iso |
en |
en |
dc.publisher |
D. Reidel Publishing Co. |
en |
dc.relation.uri |
http://adsabs.harvard.edu/abs/1984Ap%26SS.104..163S |
|
dc.relation.uri |
http://dx.doi.org/10.1007/BF00654002 |
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dc.subject |
Novae |
en |
dc.subject |
Spectrum Analysis |
|
dc.subject |
Stellar Spectrophotometry |
|
dc.subject |
Black Body Radiation |
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dc.subject |
Electron Density (Concentration) |
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dc.subject |
Emission Spectra |
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dc.subject |
Hydrogen Ions |
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dc.subject |
Line Spectra |
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dc.subject |
Stellar Envelopes |
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dc.subject |
Ion Density (Concentration) |
|
dc.title |
Spectrophotometry of Nova Coronae Austrinae, 1981 |
en |
dc.type |
Article |
en |