dc.contributor.author |
Shylaja, B. S |
|
dc.date.accessioned |
2008-09-23T10:49:55Z |
|
dc.date.available |
2008-09-23T10:49:55Z |
|
dc.date.issued |
1987 |
|
dc.identifier.citation |
IAU Symposium, No. 122, pp. 459 - 460 |
en |
dc.identifier.issn |
0074-1809 |
|
dc.identifier.uri |
http://hdl.handle.net/2248/3806 |
|
dc.description.abstract |
The binaries with subgroup WN components have been chosen, with periods ranging from 1.64 d to 21.63 d, for understanding the effect of the companion on the formation of this line. |
en |
dc.language.iso |
en |
en |
dc.publisher |
International Astronomical Union |
en |
dc.relation.uri |
http://ads.ari.uni-heidelberg.de/abs/1987IAUS..122..459S |
en |
dc.subject |
Binaries:wolf-rayet stars |
en |
dc.subject |
Wolf-Rayet Stars:binaries |
en |
dc.title |
The behaviour of λ4686 line of He II in Wolf-Rayet binaries |
en |
dc.type |
Article |
en |