dc.contributor.author |
Parthasarathy, M |
|
dc.date.accessioned |
2020-11-17T02:34:27Z |
|
dc.date.available |
2020-11-17T02:34:27Z |
|
dc.date.issued |
2017-02 |
|
dc.identifier.citation |
New Astronomy, Vol. 51, pp. 96-98 |
en_US |
dc.identifier.issn |
1384-1076 |
|
dc.identifier.uri |
http://prints.iiap.res.in/handle/2248/7034 |
|
dc.description |
Restricted Access © Elsevier B.V http://dx.doi.org/10.1016/j.newast.2016.08.018 |
en_US |
dc.description.abstract |
The discovery of K I 7699 Å line strength variations during the 1982–1984 eclipse of ε Aurigae is described. The equivalent widths and radial velocities of the K I 7699 Å line derived from spectra obtained during 1981 November–1983 July with the 2.1 m Otto Struve reflector telescope of the McDonald observatory are presented |
en_US |
dc.language.iso |
en |
en_US |
dc.publisher |
Elsevier B.V |
en_US |
dc.subject |
Stars: individual - ε Aurigae |
en_US |
dc.subject |
Stars: evolution |
en_US |
dc.subject |
Stars: circumstellar matter |
en_US |
dc.subject |
Stars: eclipsing binaries |
en_US |
dc.subject |
Stars: AGB and post-AGB |
en_US |
dc.title |
On the discovery of K I 7699 Å line strength variation during the 1982–1984 eclipse of ε Aurigae |
en_US |
dc.type |
Article |
en_US |