... Molecular Lines in Star Formation Regions the ALMA Challenge Paul Jones University of New South Wales Universidad de Chile 1 Molecular Lines in Star Formation Regions - Molecular lines trace the kinematics and chemistry (composition) of molecularclouds ...
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Ссылки http://www.atnf.csiro.au/research/workshops/2011/ALMA/Jones_ALMAworkshop.pdf -- 2370.5 Кб -- 18.05.2011 Похожие документы
... Testi, L. "Multiline spectral imaging of dense cores in the Lupus molecularcloud ... 13 coauthors "G0.253 + 0.016: A molecularcloud progenitor of an arches-like cluster ...
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Ссылки http://www.atnf.csiro.au/research/publications/CASS_Publications_2012.pdf -- 107.6 Кб -- 27.02.2013 Похожие документы
... The structure of the ISM is determined by the interplay between massive stars and the ISM: molecularclouds form massive stars; massive stars dissociate, ionize, and dynamically structure the ambient medium; the ionized medium eventually cools, recombines ...
... Between Mass-Losing Evolved Stars and MolecularClouds . The Bipolar Symmetry of Ring-Like Planetary Nebulae: . ... system is that an asymptotic giant branch (AGB) star expired within the molecularcloud (MC) containing the protosolar nebula ...
... of newly formed stars that are still embedded in their natal molecularclouds ... in the denser parts of molecularclouds with hierarchical density structure, which ... This is a rough simplification, since molecularclouds in which massive stars form ...
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Ссылки http://www.atnf.csiro.au/people/Ray.Norris/papers/n204.pdf -- 1716.8 Кб -- 07.10.2010 Похожие документы
... The motivation for a fractal-like distribution comes, in part, from observations of the ISM where both atomic and molecular hydrogen clouds exhibit hierarchical structure over a wide range of scales (see, e.g., Diamond et al. ...