Published November 15, 1980 | Version v1
Journal article Metadata-only

Multiple-shell planetary nebula formation

Creators

  • 1. Theoretical physics, Racah Institute of Physics, The Hebrew University of Jerusalem, Jerusalem, Israel

Description

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

Additional details

Publishing Information

Journal Title
Astrophys. J.
Journal Volume
241
Journal Issue
4
Series
Astrophys. J.
Journal Page Range
199-208
ISSN
0004-637X

INIS

Country of Publication
United States
Country of Input or Organization
United States
INIS RN
12614943
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Descriptors DEI
HELIUM BURNING; LUMINOSITY; MASS; PLANETARY NEBULAE; STAR EVOLUTION
Descriptors DEC
NEBULAE; OPTICAL PROPERTIES; PHYSICAL PROPERTIES; STAR BURNING