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

Published online by Cambridge University Press:  30 August 2012

Chinnathambi Muthumariappan
Affiliation:
Vainu Bappu Observatory, Indian Institute of Astrophysics, Kavalur, 635 701India email: muthu@iiap.res.in
Mudumba Parthasarathy
Affiliation:
National Astronomical Observatory of Japan 2-21-1 Osawa, Mitaka, Tokyo 181-8588, Japan McDonnell Center for the Space Sciences, Department of Physics Washington University in St. Louis, One Brookings Drive, St. Louis, MO 63130, USA Aryabhatta Research Institute of Observational Sciences Nainital - 263 129, India
Kanniah Jayakumar
Affiliation:
Vainu Bappu Observatory, Indian Institute of Astrophysics, Kavalur, 635 701India email: muthu@iiap.res.in
Manickam Appakutty
Affiliation:
Vainu Bappu Observatory, Indian Institute of Astrophysics, Kavalur, 635 701India email: muthu@iiap.res.in
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Abstract

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We present physical and chemcal properties of the disk in the eclipsing binary system ∊ 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 ∊ Aur.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2012

References

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