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    181. DISCUSSION
    ... above critical (n ) with some molecules existing in a hot, self-shielded layer close to the surface of the molecular cloud (A ... of K. At the inferred densities self-shielding of H will occur, putting molecular gas close to the surface of the cloud ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/pasa/15_2/burton/paper/node4.html -- 62.4 Кб -- 08.04.2016
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    182. Conclusions
    ... H images also enable us to determine which molecular clouds are associated with the H II region. Next Section: Acknowledgements . ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/pasa/15_1/lang/paper/node5.html -- 51.2 Кб -- 08.04.2016
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    183. Expectations of the survey
    ... Much of this star formation occurs within the dense parts of molecular clouds and complexes and may proceed as a result of instabilities within the cloud or may be triggered by energetic events near the cloud as discussed briefly below (Sect 3). ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/pasa/15_1/masheder/paper/node2.html -- 59.8 Кб -- 08.04.2016
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    184. http://www.atnf.csiro.au/whats_on/workshops/mm_science2002/talks/scurran.pdf
    ... cloud, thus decent statistics needed. 3 & 12 mm ATCA Observations All current constraints: , MNRAS 327, 1244 3 & 12 mm ATCA ... and neutron masses. 4. ... and of course, chemistry, physics and molecular cloud properties in the high redshift Universe ...
    [ Текст ]  Ссылки http://www.atnf.csiro.au/whats_on/workshops/mm_science2002/talks/scurran.pdf -- 408.4 Кб -- 26.11.2002
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    185. http://www.atnf.csiro.au/management/atuc/2004dec/docs/4.1_astro_highlights.doc
    ... Dense Molecular Gas Heated by Starburst Galaxies Cyanide chemistry is an important process in dense (>104 cm-3) molecular clouds whose presence in galaxies is tightly correlated with star-formation rate. ...
    [ Текст ]  Ссылки http://www.atnf.csiro.au/management/atuc/2004dec/docs/4.1_astro_highlights.doc -- 473.0 Кб -- 30.11.2004
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    186. Questions and Future Work
    ... How do they relate to the molecular clouds? What fraction of the ISM is in the CNM? Are there larger, warmer clouds that we are missing? ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/pasa/18_1/mccluregriffiths/paper/node4.html -- 50.9 Кб -- 08.04.2016
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    187. http://www.atnf.csiro.au/the_atnf/annual_reports/2002/17189_p65-100.pdf
    ... MHz OH sites in SNRs Star formation in molecular cloud G291.3-0.7 Kinematics of G291 ... in Carina Imaging the HCO+ molecular cloud associated with N113 SN2001ig C1085 C1086 ...
    [ Текст ]  Ссылки http://www.atnf.csiro.au/the_atnf/annual_reports/2002/17189_p65-100.pdf -- 752.5 Кб -- 14.07.2003
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    188. Parkes Radio Telescope Questions and Answers
    ... is created, as naturally as heat and light, by such things as quasars, galaxies, molecular clouds, supernovae and pulsars ... The molecular clouds in star-forming regions may need several hours of observation; the intense maser emissions from OH/IR ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/outreach/visiting/parkes/qa.html -- 58.2 Кб -- 08.04.2016
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    189. ATNF Student Symposium 2008 - Programme
    ... Following the MOPS upgrade, over 20 molecular line data cubes of a southern giant molecular cloud complex - G333 were obtained. ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/research/conferences/student_symposia/ASS2008/programme.html -- 72.8 Кб -- 11.04.2016
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    190. H I Shells
    ... We speculate that this shell was formed in a molecular cloud, where the molecular hydrogen was dissociated by the Hб  II region, RCWб 94. ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/pasa/18_1/mccluregriffiths/paper/node2.html -- 64.7 Кб -- 08.04.2016
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