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Nucleosynthesis of heavy elements: Computational experiment

โœ Scribed by I. V. Panov; S. I. Blinnikov; F. -K. Thielemann


Book ID
110126417
Publisher
Springer
Year
2001
Tongue
English
Weight
149 KB
Volume
27
Category
Article
ISSN
1063-7737

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Enhanced deuterium was not detected in the metal-poor halo stars HD 140283, the protoplanetary nebula AFGL 2688, or the Orion nebula. The Galactic Center (GC) deuterium abundance in the 50 km/s molecular cloud is (2.0-10)ร— 10 -6 and less than the local ISM D/H = (0.9-1.7)x10 -5. Thus the GC D result