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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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Bulletin of the American Astronomical Society, 34, #4
© 2002. The American Astronomical Soceity.