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-process nucleosynthesis of light elements

✍ Scribed by Lee, H. Y.; Greene, J. P.; Jiang, C. L.; Pardo, R. C.; Rehm, K. E.; Schiffer, J. P.; Wuosmaa, A. H.; Goodman, N. J.; Lighthall, J. C.; Marley, S. T.; Otsuki, K.; Patel, N.; Beard, M.; Notani, M.; Tang, X. D.


Book ID
120985900
Publisher
The American Physical Society
Year
2010
Tongue
English
Weight
711 KB
Volume
81
Category
Article
ISSN
0556-2813

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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)Γ— 10 -6 and less than the local ISM D/H = (0.9-1.7)x10 -5. Thus the GC D result