Craig J. Hogan
Published 1996-09-19Version 1
The predictions of Standard Big Bang Nucleosynthesis are summarized and compared with observations of abundances of helium in HII regions, deuterium in quasar absorbers, deuterium and helium-3 in the Galaxy, and lithium in metal-poor stars. It is concluded that the prospects are good for a precise test of the theory.
Comments: 13 pages, Latex. Contribution to the Princeton meeting, ``Critical Dialogues in Cosmology''
From the Heart of The Ghoul: C and N Abundances in the Corona of Algol B
Star formation in bar environments. II. Physical properties, age and abundances of HII regions
The electron temperatures of HII regions S 201, S 206, and S 209 : Multi-frequency GMRT observations
