AAS 201st Meeting, January, 2003
Session 89. Planetary Nebulae and Dusty Clouds
Poster, Wednesday, January 8, 2003, 9:20am-6:30pm, Exhibit Hall AB

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[89.06U] BIMA CO Observations of IRAS 07134+1005

A. Zalucha, D. Fong (University of Illinois at Urbana Champaign), M. Meixner (Space Telescope Science Institute)

IRAS 07134+1005 is a carbon rich proto-planetary nebula, which is an evolved star object transitioning between the asymptotic giant branch and planetary nebulae phases of stellar evolution. Here, we present A,B,C and D array observations of the CO J=1-0 line emission from IRAS 07134+1005 using the Berkeley-Illinois-Maryland Association (BIMA) millimeter array. We resolve its molecular envelope structure and compare it to the dust shell structures that we have previously observed at mid-infrared and optical wavelengths.

This work and Fong have been supported by NSF AST 99-81363 and Zalucha and Meixner have been also supported by NSF AST 97-33679.

The author(s) of this abstract have provided an email address for comments about the abstract: zalucha@uiuc.edu

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