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    121. Staff Directory
    ... Star and planet formation; jets/outflows/turbulence in molecular clouds; dust processing, gas and ice signatures of accretion ... of diffuse, dense, star-forming clouds; multi-wavelength spectroscopy; atomic and molecular astrophysics; astrobiology ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/institute/smo/general-information/research-staff-directory -- 80.2 Кб -- 11.04.2016
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    122. HST this week: 229
    ... This proposal focuses on 252 sources within the Orion A molecular cloud, the complex that includes the Orion Nebula Cluster. ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/~inr/thisweek1/2009/thisweek229.html -- 11.5 Кб -- 05.10.2009
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    123. http://www.stsci.edu/~inr/drafts/twhyd.ps
    ... W. M. Keck Foundation. -- 2 -- is not associated with a parent molecular cloud, but the presence of a substantial gas­ and dust ...
    [ Текст ]  Ссылки http://www.stsci.edu/~inr/drafts/twhyd.ps -- 799.8 Кб -- 08.06.2007
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    124. HST this week: 233
    ... 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/thisweek1/2012/thisweek233.html -- 15.3 Кб -- 22.08.2012
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    125. http://www.stsci.edu/ftp/observing/status_reports/old_reports_94/hst_status_11_29_94
    ... disks Around Young Stellar Objects) The WF/PC-2 was used to make images of the disk around the young proto-star SAO76411A located in the Taurus molecular cloud to learn about its physical properties such as albedo, particle size, and spatial distribution ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/ftp/observing/status_reports/old_reports_94/hst_status_11_29_94 -- 10.0 Кб -- 29.11.1994
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    126. HST this week: 097
    ... 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/thisweek1/2014/thisweek097.html -- 19.7 Кб -- 08.04.2014
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    127. HST this week: 013
    ... Brown dwarfs are objects that form in the same manner as stars, by gravitational collapse within molecular clouds, but which do not accrete sufficient mass to raise the central temperature above ~2 million Kelvin and ignite hydrogen fusion. ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/~inr/thisweek1/2014/thisweek013.html -- 19.4 Кб -- 22.01.2016
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    128. HST this week: 303
    ... A Direct CO/H2 Abundance Measurement in Diffuse and Translucent LMC and SMC Molecular Clouds . 12587 . ... 12978 . Daniel E. Welty, University of Chicago . Properties of Diffuse Molecular Gas in the Magellanic Clouds . 12995 . ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/~inr/thisweek1/2012/thisweek303.html -- 21.3 Кб -- 24.11.2014
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    129. HST this week: 067
    ... Small Magellanic Cloud Ultraviolet Dust Extinction: A Focused Study of Four Sightlines Near a Molecular Cloud with Variable 2175 A bumps . 14227 . ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/~inr/thisweek1/2016/thisweek067.html -- 22.2 Кб -- 09.03.2016
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    130. Author Query Results
    ... Molecular oxygen in the №Б Ophiuchi cloud . 83 . 2007ApJ...658L..45L . ... Volk, Kevin; Geballe, T. R.; Mehringer, David M. W51 IRS 2: A Massive Jet Emerging from a Molecular Cloud into an H II Region ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/~volk/kvolk_refereed_papers.html -- 289.4 Кб -- 26.09.2014
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