BIMA CO Observations of IRAS 07134+1005

Details BIMA CO Observations of IRAS 07134+1005 BIMA CO Observations of IRAS 07134+1005

Dec 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aas...201.8906z&link_type=abstract

American Astronomical Society, 201st AAS Meeting, #89.06; Bulletin of the American Astronomical Society, Vol. 34, p.1253

Astronomy and Astrophysics

Astronomy

Scientific paper

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.

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