Published 1975 | Version v1
Book

Interstellar isotopic ratios, stellar mass losses and galactic evolution

  • 1. Observatoire de Meudon, France

Description

A study of presently available data shows that the 12C/13C ratio in the interstellar matter is about 40, rather than 89 as in the solar system, which has the isotopic composition of the interstellar matter 4.6 x 109 years ago. Mass loss by evolved stars and possibly novae is responsible for relative enrichment in 13C. Isotopes of CNO seem to be very promising tools for the study of galactic evolution. 7 refs

Additional details

Publishing Information

Publisher
Springer-Verlag.
Imprint Place
New York
Imprint Title
H II regions and related topics
Imprint Pagination
p. 356-359.

Conference

Title
Symposium on H II regions and related topics.
Dates
13 Jan 1975.
Place
Mittelberg, Kleinwalsertal, Austria.

INIS

Country of Publication
United States
Country of Input or Organization
United States
INIS RN
8297552
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Resource subtype / Literary indicator
Conference
Descriptors DEI
CARBON; COSMOCHEMISTRY; GALACTIC EVOLUTION; INTERSTELLAR SPACE; ISOTOPE RATIO; MASS; MASS TRANSFER; STAR EVOLUTION
Descriptors DEC
CHEMISTRY; ELEMENTS; NONMETALS; SPACE

Optional Information

Notes
Imprint:See CONF-750142--.