dc.contributor.author |
Giridhar, S |
|
dc.date.accessioned |
2008-09-22T12:09:01Z |
|
dc.date.available |
2008-09-22T12:09:01Z |
|
dc.date.issued |
1987-05 |
|
dc.identifier.citation |
Revista Mexicana de Astronomia y Astrofisica , Vol. 14, No. 2, pp. 431 - 434 |
en |
dc.identifier.issn |
0185-1101 |
|
dc.identifier.uri |
http://hdl.handle.net/2248/3769 |
|
dc.description.abstract |
Fine analysis of the southern Cepheid β Dor has been conducted at different phases with the aim to derive atmospheric parameters at those phases. Atmospheric abundances have been derived for Fe group elements and s-process elements. The derived parameters of β Dor are compared with earlier estimates. |
en |
dc.language.iso |
en |
en |
dc.publisher |
Universidad Nacional Autonoma De Mexico |
en |
dc.relation.uri |
http://adsabs.harvard.edu/abs/1987RMxAA..14..431G |
en |
dc.subject |
Star Abundance |
en |
dc.subject |
Cepheid variables |
en |
dc.subject |
Stellar atmospheres |
en |
dc.subject |
Stellar spectra |
en |
dc.subject |
Atmospheric models |
en |
dc.subject |
Electron scattering |
en |
dc.subject |
Line spectra |
en |
dc.title |
Spectroscopic studies of the southern Cepheid β Dor |
en |
dc.type |
Article |
en |