... HISA gas traces the small fraction of molecularcloud gas that is atomic, unless the ... of the shock, where it forms molecularclouds and then the massive stars that define ...
... are: (1) the formation and lifetimes of molecularclouds; (2) disk-halo interaction ... field studies of supernova remnants (SNRs), molecularclouds, and H II regions; (3 ...
... Dark Molecular Gas in the Pegasus-Pisces Region In the last decade, the importance of a largely ignored component of molecularclouds (dubbed somewhat misleadingly as dark molecular gas) has become a source of study and debate over its abundance and role ...
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Ссылки http://www.naic.edu/vscience/schedule/tpfiles/MagnanitagA3021tp.pdf -- 47.3 Кб -- 03.10.2015 Похожие документы
... Galactic Total Time Requested: 28 Hours Minimum Useful Time: 3 hours Proposal Title: Zeeman Measurements of OH Spectral lines in Starless Clouds ABSTRACT: The fragmentation of molecularclouds and the formation of cores are still intensely debated issues ...
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Ссылки http://www.naic.edu/vscience/schedule/tpfiles/HezarehtagA2708tp.ps -- 87.2 Кб -- 01.10.2013 Похожие документы
... and Goldsmith, P.F., Density Structure in Giant MolecularCloud Cores , Astrophys ... P. F., The Clumpy Structure of MolecularClouds In "Amazing Light a Volume Dedicated ...
... the gas is mostly H 2 ( f n = 0.01), it has typical molecularcloud temperatures ... are many HISA clouds containing CO, but either the atomic/molecular fraction is not ... of HISA tracing a small, fixed fraction of atomic gas in molecularclouds ...