Measurements of 3He in Galactic HII regions and planetary nebulae

Details Measurements of 3He in Galactic HII regions and planetary nebulae Measurements of 3He in Galactic HII regions and planetary nebulae

Apr 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010iaus..268...81b&link_type=abstract

Light Elements in the Universe, Proceedings of the International Astronomical Union, IAU Symposium, Volume 268, p. 81-90

Mathematics

Logic

2

Cosmology: Cosmological Parameters, The Galaxy: Abundances, Evolution, Ism: Abundances, Evolution, Hii Regions, Stars: Agb, Post-Agb

Scientific paper

The cosmic abundance of the 3He isotope has important implications for many fields of astrophysics. We are using the 8.665 GHz hyperfine transition of 3He+ to determine the 3He/H abundance in Milky Way H ii regions and planetary nebulae. Here we review the 30 year history of our 3He program, report on its current status, and describe our future plans.

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