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    191. http://www.stsci.edu/jwst/doc-archive/white-papers/JWST_Solar_System.pdf
    ... the solar system formed, and this information can be compared with and placed in the context of compositional studies of molecular clouds and the interstellar medium to better constrain the cycle of matter in the galaxy (Gardner et al., 2006) (figure 2 ...
    [ Текст ]  Ссылки http://www.stsci.edu/jwst/doc-archive/white-papers/JWST_Solar_System.pdf -- 518.7 Кб -- 05.02.2013
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    192. Marshall Perrin's Research
    ... young stars play a major role in star formation, both by removing angular momentum from circumstellar disks (and thus enabling accretion to continue), and by driving turbulence in molecular clouds (and thereby regulating the efficiency of star formation ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/~mperrin/research.shtml -- 15.4 Кб -- 10.04.2016
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    193. http://www.stsci.edu/institute/conference/stellar-imf/Schedule.pdf
    ... Offner ­ Protostellar Outflows and Their Impact on the IMF Robert Gutermuth ­ An LMT/AzTEC Survey for Dense Cores in the MonR2 Giant Molecular Cloud LU N C H Chair: Mario Gennaro Morten Andersen ­ The Low-Mass IMF of Westerlund 1, the Most Massive Young ...
    [ Текст ]  Ссылки http://www.stsci.edu/institute/conference/stellar-imf/Schedule.pdf -- 100.7 Кб
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    194. HST and the Distant Universe
    ... G. P. Di Benedetto . Cosmological Molecular Clouds . D. Puy and M. Signore . payne@stsci.edu. ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/stsci/meetings/shst2/node3.html -- 3.0 Кб -- 15.06.2005
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    195. http://www.stsci.edu/stsci/meetings/planets/abs/prog30.html
    ... A very young "blister" H II region, with an associated embedded cluster actively being excavated from its parent molecular cloud, appears necessary to show circumstellar ionization and absorption regions before the harsh nebular environment can sweep the ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/stsci/meetings/planets/abs/prog30.html -- 3.6 Кб -- 22.10.1996
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    196. Imaging of the Supernova Remnant Cassiopeia A with the Multiband Imaging
    ... The IR images also show a region in which the SNR forward shock appears to be propagating into a ~650 Msolar molecular cloud. ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/~kgordon/papers/2004ApJS..154..290H.html -- 4.8 Кб -- 21.01.2016
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    197. Starburst and Galaxy Evolution
    ... Modelling the pan-spectral energy distribution of starburst galaxies: I. The role of ISM pressure and the molecular cloud dissipation timescale . ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/science/starburst99/CCGI/Preprints2005.cgi -- 6.7 Кб -- 10.04.2016
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    198. The 24 Micron View of Embedded Star Formation in NGC 7129
    ... Most of the pre-main-sequence candidates are associated with the densest part of the molecular cloud surrounding the photoionization region, indicating active star formation over a broad area outside the central cluster. ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/~kgordon/papers/2004ApJS..154..379M.html -- 4.5 Кб -- 21.01.2016
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    199. HST this week: 299
    ... Brown dwarfs are failed stars - objects that form like stars, by gravitational collapse within giant molecular clouds, but which have insufficient mass to raise the central temperature above 10 7 K, and which therefore are unable to ignite hydrogran ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/~inr/thisweek1/2015/thisweek299.html -- 19.6 Кб -- 12.11.2015
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    200. HST this week: 053
    ... S. Thomas Megeath, University of Toledo . A Snapshot WFC3 IR Survey of Spitzer/Hershel-Identified Protostars in Nearby Molecular Clouds . 14199 . ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/~inr/thisweek1/2016/thisweek053.html -- 19.5 Кб -- 04.03.2016
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