dc.contributor.author |
Mallik, S. G. V |
|
dc.date.accessioned |
2008-12-18T15:19:09Z |
|
dc.date.available |
2008-12-18T15:19:09Z |
|
dc.date.issued |
1982-03 |
|
dc.identifier.citation |
Journal of Astrophysics and Astronomy, Vol. 3, pp. 39 - 61 |
en |
dc.identifier.issn |
0250-6335 |
|
dc.identifier.uri |
http://hdl.handle.net/2248/4128 |
|
dc.description |
Open Access |
|
dc.description.abstract |
H-alpha is investigated spectroscopically in order to gain information on the properties of expanding chromospheres of late G and K supergiants. Spectra of 23 stars brighter than V equals 6.0 are obtained at dispersions of 4-10 A/mm using the coude and the coude-echelle spectrographs at the 102-cm telescope of Kavalur Observatory. H-alpha profiles are computed theoretically using radiative transfer in spherically symmetric expanding atmospheres covering a large range of integrated optical depths. These are then compared with the characteristics of the observed line in the program stars. The analysis reveals that the H-alpha line is formed in a region with velocity increasing outward. The computer equivalent widths and line core displacements are matched with those observed to obtain hydrogen column densities and expansion velocities. |
en |
dc.language.iso |
en |
en |
dc.publisher |
Indian Academy of Sciences |
en |
dc.relation.uri |
http://adsabs.harvard.edu/abs/1982JApA....3...39M |
en |
dc.rights |
© Indian Academy of Sciences |
|
dc.subject |
G Stars |
en |
dc.subject |
H Alpha Line |
en |
dc.subject |
K Stars |
en |
dc.subject |
Late-Types Stars |
en |
dc.subject |
Stellar Mass Ejection |
en |
dc.subject |
Stellar Spectra |
en |
dc.subject |
Supergiant Stars |
en |
dc.subject |
Chromosphere |
en |
dc.subject |
Spectrograms |
en |
dc.subject |
Stellar Winds |
en |
dc.subject |
Mass Loss |
|
dc.title |
A study of the H-alpha line in late G and K supergiants |
en |
dc.type |
Article |
en |