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Spectroscopy of the Ionizing Sources of UC HII Regions
Published online by Cambridge University Press: 30 March 2016
Abstract
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The utility of near-infrared, spectroscopic studies of central ionizing sources of UC HII regions is presented, in conjunction with a recently available, sophisticated atmospheric code, to constrain the physical conditions and environment of very massive stars at extremely early stages of evolution.
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- II. Joint Discussions
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- Copyright © Astronomical Society of Pacific 2002