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    81. Ron Allen
    ... Large-scale Properties of the ISM from observations of nearby galaxies: structure and physics of cold molecular clouds (Loinard); dust content from background galaxy counts and colors (Gonzalez); PDR models for the HI content of galaxies (Smith). ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/stsci/meetings/jamb98/node2.html -- 3.4 Кб -- 24.03.1998
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    82. Dust Around Stars
    ... Where there are hot stars in and around molecular clouds the dust gets heated to much higher temperatures than in the general diffuse interstellar medium (say 50 to 150 K), and its radiation can be detected down to around a wavelength of 10 microns or so. ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/~volk/dust.html -- 6.7 Кб -- 27.05.2014
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    83. HST this week: 182
    ... revealing several massive OB clusters lying within a giant molecular cloud that is still at an early stage of disruption ... reddened, however, due to both dust within the parent molecular cloud and foreground material along the line of sight, which ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/~inr/thisweek1/2008/thisweek182.html -- 15.5 Кб -- 21.07.2008
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    84. The Mass Accretion Rates of Intermediate-Mass T Tauri Stars
    ... We argue that reddening laws with these characteristics may well be representative of cold, dense molecular clouds. ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/~kgordon/papers/2004AJ....128.1294C.html -- 5.5 Кб -- 21.01.2016
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    85. Target Category and Target Description [Description]
    ... Herbig-Haro Object . Cometary Nebula . Planetary Nebula . Molecular Cloud . HII Region . Bipolar Outflow . Reflection Nebula . ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/ftp/documents/p2pi/HTMLjavahelpCy20/ch03_targ_fixed04.html -- 130.5 Кб -- 31.05.2012
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    86. http://www.stsci.edu/institute/conference/may_symp/supportingFiles/poster71
    ... of Toronto) STScI May Symposium 2006 Overview The giant molecular clouds (GMCs) are the places where massive stars actively ...
    [ Текст ]  Ссылки http://www.stsci.edu/institute/conference/may_symp/supportingFiles/poster71 -- 578.7 Кб -- 11.05.2006
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    87. GHRS Instrument Science Report 091: . Summary of GHRS Documentation
    ... The Translucent Molecular Clouds toward HD 154368. I. Extinction, Abundances, and Depletions" . ... Ultraviolet DIB at 1369 е Arising in Molecular Clouds" . Gnacinski, P., Sikorski, J., and Kacmarczyk, G. 1997, Acta Astron. ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/hst/ghrs/documents/isrs/ghrs_isr091.html -- 69.2 Кб -- 11.04.2016
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    88. Talks
    ... where the materials that were present in the parent molecular cloud are processed to various degrees prior to incorporation ... Interstellar grains in molecular clouds are coated with icy mantles once the visual extinction exceeds about 3 magnitudes ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/institute/conference/volatile/talks -- 58.8 Кб -- 10.04.2016
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    89. http://www.stsci.edu/hst/proposing/docs/exp_abstract-catalogs/Cycle23-Approved-Programs.pdf
    ... Dust Extinction: A Focused Study of Four Sightlines Near a Molecular Cloud with Variable 2175 A bumps Probing Extended Star ...
    [ Текст ]  Ссылки http://www.stsci.edu/hst/proposing/docs/exp_abstract-catalogs/Cycle23-Approved-Programs.pdf -- 152.6 Кб
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    90. http://www.stsci.edu/institute/smo/events/colloquia/2008/ColloquiaJune4Fall.pdf
    ... June 4, 2008 Michael Fall, Space Telescope Science Institute This talk will present a comprehensive picture of the life cycles of star clusters, from their birth in molecular clouds to their dissolution in the field (unclustered) stellar population ...
    [ Текст ]  Ссылки http://www.stsci.edu/institute/smo/events/colloquia/2008/ColloquiaJune4Fall.pdf -- 204.2 Кб -- 05.02.2013
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