dc.contributor.author |
Muthumariappan, C |
|
dc.contributor.author |
Parthasarathy, M |
|
dc.contributor.author |
Jayakumar, K |
|
dc.contributor.author |
Appakutty, M |
|
dc.date.accessioned |
2012-09-04T13:33:47Z |
|
dc.date.available |
2012-09-04T13:33:47Z |
|
dc.date.issued |
2012-08 |
|
dc.identifier.citation |
Proceedings of the International Astronomical Union, Vol. 283, pp. 454-455 |
en |
dc.identifier.isbn |
9781107019836 |
|
dc.identifier.uri |
http://hdl.handle.net/2248/5884 |
|
dc.description |
Restricted Access |
en |
dc.description.abstract |
We present physical and chemcal properties of the disk in the eclipsing binary system ɛ Aur by solving 2D radiative transfer problem. We also present preliminary results of our high resolution spectroscopic monitoring of K I, Na, and Hα line profiles variation during the totality phase of the recent eclipse of ɛ Aur. |
en |
dc.language.iso |
en |
en |
dc.publisher |
Cambridge University Press |
en |
dc.relation.ispartofseries |
IAU Symposium No. 283 |
|
dc.relation.uri |
http://dx.doi.org/10.1017/S1743921312011891 |
en |
dc.rights |
© International Astronomical Union |
en |
dc.subject |
Stars: binaries: eclipsing |
en |
dc.subject |
Stars: circumstellar matter |
en |
dc.subject |
Radiative transfer |
en |
dc.title |
ɛ Aur in eclipse: Post-AGB primary and disk-shaped secondary |
en |
dc.type |
Article |
en |