Published June 15, 1974 | Version v1
Journal article Metadata-only

Some recent results from galactic and stellar evolution theory

Creators

  • 1. Department of Space Physics and Astronomy, Rice University, Houston, Texas

Description

Recent progress in stellar and galactic evolution theory give excellent agreement between observational abundances and the theoretical yields for elements heavier than helium. This includes the secondary production of 14N and the variation of N/O over the face of MiOl which was observed by Searle. Subject headings: abundances - galactic structure - nucleosynthesis - stellar evolution

Additional details

Additional titles

Augmented title (English)
Direct application, elements heavier than helium, observed by Searle

Identifiers

DOI
10.1086/152918;

Publishing Information

Journal Title
The Astrophysical Journal
Journal Volume
190
Journal Issue
3
Series
Astrophys. J.
Journal Page Range
605
ISSN
0004-637X

INIS

Country of Publication
United States
Country of Input or Organization
United States
INIS RN
6159402
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Descriptors DEI
CHEMICAL COMPOSITION; COSMOCHEMISTRY; GALACTIC EVOLUTION; HYDROGEN; NITROGEN; NUCLEOSYNTHESIS; OXYGEN; STAR EVOLUTION
Descriptors DEC
CHEMISTRY; ELEMENTS; NONMETALS

Optional Information

Notes
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