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Spitzer/MIPS Imaging of the Extremely Extended Dust Shell(s) around R Hya

Published online by Cambridge University Press:  15 December 2006

Angela K. Speck ,
Toshiya Ueta  and
the MIRIAD team
Angela K. Speck
Affiliation:
Physics & Astronomy, University of Missouri, Columbia, MO 65211, USA email: speckan@missouri.edu
Toshiya Ueta
Affiliation:
NASA Ames Research Center/USRA SOFIA Office, Mail Stop 211-3, Moffett Field, CA 94035.
the MIRIAD team
Affiliation:
R. Stencel (University of Denver), R. Gehrz (University of Minnesota), W. Latter (IPAC), M. Meixner (STScI), M. Elitzur (University of Kentucky), F. Herwig (LANL), H. Izumiura (NAOJ), M. Matsuura (Queen's University, Belfast), R. Szczerba (NCAC), M. Steffen (AIP), A. Zijlstra (University of Manchester)
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Abstract

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We present Spitzer/MIPS far-infrared (FIR) mapping of O-rich AGB star, R Hya.

Keywords

stars: AGB and post-AGBstars: circumstellar matterstars: mass loss
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2 , Symposium S234: Planetary Nebulae in our Galaxy and Beyond , April 2006 , pp. 515 - 516
Copyright
© 2006 International Astronomical Union