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Uncertainties in nebular helium abundances

Published online by Cambridge University Press:  23 April 2010

Evan D. Skillman*
Affiliation:
Astronomy Department, University of Minnesota, 116 Church St. SE, Minneapolis, MN, USA email: [email protected]
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Abstract

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Efforts to determine the primordial helium abundance via observations of metal poor HII regions have been limited by significant uncertainties. Because of a degeneracy between the solutions for density and temperature, the precision of the helium abundance determinations is limited. Spectra from the literature are used to show the effects of new atomic data and to demonstrate the challenges of determining precise He abundances. Several suggestions are made for meeting these challenges.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2010

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