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    91. http://www.stsci.edu/ftp/observing/status_reports/old_reports_99/hst_status_03_31_99
    ... The target is a bright soft X-ray source in the direction of the R CrA molecular cloud. ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/ftp/observing/status_reports/old_reports_99/hst_status_03_31_99 -- 7.0 Кб -- 31.03.1999
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    92. http://www.stsci.edu/ftp/observing/status_reports/old_reports_96/hst_status_10_28_96
    ... 1.16 Completed GHRS/1 6723 (Physical Conditions Near High Galactic = Latitude Molecular Clouds) The High Resolution Spectrograph (Side One) was used to make = observations of background star HD89688 whose light passes through a high = galactic molecular ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/ftp/observing/status_reports/old_reports_96/hst_status_10_28_96 -- 10.9 Кб -- 28.10.1996
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    93. http://www.stsci.edu/science/preprints/prep1563/prep1563.pdf
    ... formation about 2.5±0.5 Myr ago, from a molecular cloud which is no longer present ... ionizing the surface of a background molecular cloud, thus pro ducing the Thermal ... providing the heating source for the nearby molecular cloud, Lcloud 107 L ...
    [ Текст ]  Ссылки http://www.stsci.edu/science/preprints/prep1563/prep1563.pdf -- 1758.0 Кб -- 26.11.2002
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    94. Summary of GHRS Documentation at STScI and a GHRS Bibliography
    ... 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/ftp/instrument_news/GHRS/Ghrs_isr/ghrs_isr091/ghrs_isr091.html -- 64.7 Кб -- 12.05.2000
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    95. IAU Symposium 258 Poster Abstracts
    ... recognized as a valuable new laboratory for studying molecular cloud properties during the earliest stages of star formation ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/institute/conference/iau258/posters -- 105.2 Кб -- 10.04.2016
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    96. Science Results from Pan-STARRS1
    ... Mr. Chien-Cheng Lin (National Central University) . Most if not all stars formed clustered in molecular clouds. ... of the sky; a catalog of distances to high-latitude molecular clouds; and the unveiling of a new shell of dust in the Orion ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/institute/conference/panstarrs1/talksList -- 65.9 Кб -- 10.04.2016
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    97. HST this week: 203
    ... 12978 . Daniel E. Welty, University of Chicago . Properties of Diffuse Molecular Gas in the Magellanic Clouds . 12982 . ... that form like stars, by gravitational collapse within giant molecular clouds, but which have insufficient mass to raise the ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/~inr/thisweek1/2013/thisweek203.html -- 18.3 Кб -- 13.11.2013
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    98. Phase I Proposals
    ... USA . Physical conditions near high galactic latitude molecular clouds . Matthew . Bobrowsky . SNAP . ... ISM . Johns Hopkins University . USA . Search for Interstellar Water in Translucent Molecular Clouds . Keith . Noll . GO . ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/hst/proposing/exp_abstract-catalogs/cy6-approved -- 109.2 Кб -- 11.04.2016
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    99. HST this week: 327
    ... 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/thisweek327.html -- 13.3 Кб -- 19.01.2010
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    100. http://www.stsci.edu/~marel/decadal/sc/282.pdf
    ... the gas mass is in dense clumps, and how the mass function of molecular clouds compares with that of recently formed clusters ...
    [ Текст ]  Ссылки http://www.stsci.edu/~marel/decadal/sc/282.pdf -- 1812.0 Кб -- 19.02.2009
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