Skip to main content
U.S. Department of Energy
Office of Scientific and Technical Information

Multiple-shell planetary nebula formation

Journal Article · · Astrophys. J.; (United States)
DOI:https://doi.org/10.1086/158456· OSTI ID:6522663
Predictions of the combination of our recent model for the formation of planetary nebulae (due to a diverging pulsational instability) together with nuclear-burning shell flashing, with regard to formation of multiple shells, are explored and discussed.
Research Organization:
Theoretical physics, Racah Institute of Physics, The Hebrew University of Jerusalem, Jerusalem, Israel
OSTI ID:
6522663
Journal Information:
Astrophys. J.; (United States), Journal Name: Astrophys. J.; (United States) Vol. 241:4; ISSN ASJOA
Country of Publication:
United States
Language:
English

Similar Records

Hydrogen shell game - pulsational instabilities in hydrogen shell-burning planetary nebula nuclei
Journal Article · Mon Oct 31 23:00:00 EST 1988 · Astrophys. J.; (United States) · OSTI ID:6534537

Miras and planetary nebula formation
Journal Article · Wed Nov 14 23:00:00 EST 1979 · Astrophys. J.; (United States) · OSTI ID:5731420

Helium shell game - nonradial g-mode instabilities in hydrogen-deficient planetary nebula nuclei
Journal Article · Tue Jul 01 00:00:00 EDT 1986 · Astrophys. J.; (United States) · OSTI ID:7259542