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    131. http://www.atnf.csiro.au/pasa/15_1/stark/paper.pdf
    ... It is important to realise that every cloud has a translucent layer: the edges of dark clouds, giant molecular clouds, and, in the ultimate sense, the edge of every clump is a translucent region. ...
    [ Текст ]  Ссылки http://www.atnf.csiro.au/pasa/15_1/stark/paper.pdf -- 356.9 Кб -- 14.05.1998
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    132. http://www.atnf.csiro.au/pasa/15_1/chu/paper.pdf
    ... in the LMC The structure of the ISM is determined by the interplay between massive stars and the ISM: molecular clouds form massive stars; massive stars dissociate, ionise, and dynamically structure the ambient medium; the ionised medium eventually cools ...
    [ Текст ]  Ссылки http://www.atnf.csiro.au/pasa/15_1/chu/paper.pdf -- 263.3 Кб -- 14.05.1998
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    133. Types of Stars
    ... Stars form in dense molecular clouds within galaxies. ... Protostars form when sections of giant molecular clouds start to collapse. ... The gravitational collapse of a giant molecular cloud does not result in a single ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/outreach/education/senior/cosmicengine/stars_types.html -- 74.9 Кб -- 11.04.2016
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    134. The Target Positions
    ... Searching for good candidates for high-density molecular clouds is not an easy task in the LMC. ... which is too coarse to find high density clumps (nevertheless, we observed towards Molecular Cloud Complex 35, no. 7 in Table 1 ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/pasa/14_3/osterberg/paper/node3.html -- 54.8 Кб -- 08.04.2016
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    135. http://www.atnf.csiro.au/research/publications/ATNF_Publications_2009.pdf
    ... Molecular clouds towards RCW49 and Westerlund 2: evidence for cluster formation ... Molecular line mapping of the giant molecular cloud associated with RCW 106. III. ...
    [ Текст ]  Ссылки http://www.atnf.csiro.au/research/publications/ATNF_Publications_2009.pdf -- 85.2 Кб -- 03.03.2010
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    136. ATNF Colloquium
    ... to study carbon in all its forms, as it cycles from molecular clouds into stars and back to the interstellar medium --- an ... We will directly witness the formation and destruction of molecular clouds. ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/news/news.php?action=show_item&item_id=723 -- 27.1 Кб -- 01.03.2014
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    137. Jo Dawson's Homepage
    ... Way and nearby galaxies, and in particular on the mechanisms by which the atomic medium is processed into molecular clouds ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/people/Joanne.Dawson/ -- 26.4 Кб -- 09.04.2016
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    138. ATNF Colloquium
    ... In particular, Herschel is unveiling the filamentary structure and molecular cloud constituents of the ISM where . ... HOBYS has already proven fruitful with many clear examples of high-mass star formation in nearby molecular cloud complexes. ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/news/news.php?action=show_item&item_id=1059 -- 28.4 Кб -- 01.03.2014
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    139. ATNF Colloquium
    ... star formation: (1) magnetic support of molecular clouds against gravity . ... in molecular clouds will then be used to apply the tests, and the results . ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/news/news.php?action=show_item&item_id=503 -- 27.3 Кб -- 01.03.2014
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    140. ATNF Publications 2006
    ... Molecular line mapping of the giant molecular cloud associated with RCW 106. ... A. & FUKUI, Y. "Detection of molecular clouds in the Magellanic Bridge: candidate ... L.K. "Evolution of H II regions in hierarchically structured molecular clouds ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/research/publications/AT2006.html -- 97.8 Кб -- 08.04.2016
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