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

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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

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