Spectrophotometry of Nova Coronae Austrinae, 1981

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
dc.format.mimetype	application/pdf
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
dc.subject	Novae	en
dc.subject	Spectrum Analysis
dc.subject	Stellar Spectrophotometry
dc.subject	Black Body Radiation
dc.subject	Electron Density (Concentration)
dc.subject	Emission Spectra
dc.subject	Hydrogen Ions
dc.subject	Line Spectra
dc.subject	Stellar Envelopes
dc.subject	Ion Density (Concentration)
dc.title	Spectrophotometry of Nova Coronae Austrinae, 1981	en
dc.type	Article	en