Hostname: page-component-78c5997874-mlc7c Total loading time: 0 Render date: 2024-11-06T02:12:07.095Z Has data issue: false hasContentIssue false
  • English
  • Français

The Molecular Morphology of Evolved Stars

Published online by Cambridge University Press:  26 May 2016

D. Fong ,
M. Meixner ,
E. C. Sutton  and
W. J. Welch
D. Fong
Affiliation:
University of Illinois, 1002 W. Green St., Urbana, Il. 61801, USA
M. Meixner
Affiliation:
University of Illinois, 1002 W. Green St., Urbana, Il. 61801, USA
E. C. Sutton
Affiliation:
University of Illinois, 1002 W. Green St., Urbana, Il. 61801, USA
W. J. Welch
Affiliation:
University of California, Radio Astronomy Lab, Berkeley, Ca. 94720

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

We present 12CO J=1-0 observations of a small sample of evolved stars to investigate the evolution of the molecular envelope from the AGB phase to the formation of the PN.

Type
Part V: Dust and Molecules in Planetary Nebulae
Information
Symposium - International Astronomical Union , Volume 209: Planetary Nebulae: Their Evolution and Role in the Universe , 2003 , pp. 273 - 274
Copyright
Copyright © Astronomical Society of the Pacific 2003