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The Structure and Evolution of Early Cosmological H<scp>ii</scp>Regions
ASTROPHYSICAL JOURNAL, no. 2 (2004): 631-645
摘要
We study the formation and evolution of H II regions around the first stars formed at redshifts z = 10-30. We use a one-dimensional Lagrangian hydrodynamics code that self-consistently incorporates radiative transfer and nonequilibrium primordial gas chemistry. The star-forming region is defined as a spherical dense molecular gas cloud wi...更多
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