Hostname: page-component-7bb8b95d7b-s9k8s Total loading time: 0 Render date: 2024-09-18T01:54:22.493Z Has data issue: false hasContentIssue false
  • English
  • Français

Oscillating Stars (MIRAS), Mass Loss and Formation of Planetary Nebulae (PN)

Published online by Cambridge University Press:  22 September 2016

I. Tuchman ,
N. Sack  and
Z. Barkat
I. Tuchman
Affiliation:
The Hebrew University of Jerusalem, Israel
N. Sack
Affiliation:
The Hebrew University of Jerusalem, Israel
Z. Barkat
Affiliation:
The Hebrew University of Jerusalem, Israel

Extract

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 report some results of an extensive study of dynamically and/or pulsationally unstable stellar envelopes at the red giant stage.

Type
Session VII: The Origin of Planetary Nebulaesession VII the Origin of Planetary Nebulae
Information
Symposium - International Astronomical Union , Volume 76: Planetary Nebulae , 1978 , pp. 323
Copyright
Copyright © Reidel 1978