dc.contributor.author |
Prabhu, T. P |
|
dc.contributor.author |
Anupama, G. C |
|
dc.date.accessioned |
2008-09-23T14:27:29Z |
|
dc.date.available |
2008-09-23T14:27:29Z |
|
dc.date.issued |
1987-03 |
|
dc.identifier.citation |
Astrophysics and Space Science , Vol. 131, No. 1 - 2, pp. 479 - 484 |
en |
dc.identifier.issn |
0004-640X |
|
dc.identifier.uri |
http://hdl.handle.net/2248/3839 |
|
dc.description.abstract |
Optical spectroscopic data of the nova LW Serpentis 1978, covering its diffuse-enhanced phase until the onset of the forbidden O I line flash, were obtained at the Vainu Bappu Observatory, Kavalur, between March 10 and April 7, 1978. Emission lines, covering a range of 4000-8700 A at dispersions ranging from 83-675 A/mm, steadily increased during the observation period, with highest increases for H-alpha and O I 8446 A. A mean absorption velocity of -1303 + or - 46 km/s is deduced, and the present spectral evolution is consistent with those of fast novae such as NQ Vul 1976. |
en |
dc.language.iso |
en |
en |
dc.publisher |
Kluwer Academic Publishers |
en |
dc.relation.uri |
http://dx.doi.org/10.1007/BF00668129 |
en |
dc.subject |
Novae |
en |
dc.subject |
Radiant flux density |
en |
dc.subject |
Stellar spectrophotometry |
en |
dc.subject |
Visible spectrum |
en |
dc.subject |
Oxygen |
en |
dc.subject |
Spectral energy distribution |
en |
dc.subject |
Spectral resolution |
en |
dc.subject |
Spectrum analysis |
en |
dc.title |
The optical spectrum of nova LW Serpentis 1978 |
en |
dc.type |
Article |
en |