ɛ Aur in eclipse: Post-AGB primary and disk-shaped secondary

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/5884

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DC Field	Value	Language
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
Appears in Collections:	IIAP Publications

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