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    71. http://www.stsci.edu/~kgordon/papers/PS_files/hd197.ps.gz
    ... possibly on the edge of a molecular cloud/star formation region including Lynds 1036 ... the images mark the edge of a molecular cloud which has been mapped in CO (Dobashi ...
    [ Текст ]  Ссылки http://www.stsci.edu/~kgordon/papers/PS_files/hd197.ps.gz -- 53.5 Кб -- 23.04.2003
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    72. Institute for Planets and Life
    ... regions of a protoplanetary disk or inheritance from the parent molecular cloud ... of its water, and perhaps other primordial ices, from the parent molecular cloud ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/institute/smo/ipl/abstracts -- 89.3 Кб -- 10.04.2016
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    73. http://www.stsci.edu/ftp/observing/status_reports/old_reports_96/hst_status_11_19_96
    ... 1.4 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 HD298497 whose light passes through a = high galactic molecular ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/ftp/observing/status_reports/old_reports_96/hst_status_11_19_96 -- 4.7 Кб -- 19.11.1996
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    74. http://www.stsci.edu/ftp/observing/status_reports/old_reports_95/hst_status_11_07_95
    ... 1.3 Completed GHRS/1/2 5739 (Ultraviolet Spectroscopy of High Latitude = Molecular Cloud: Carryover) The High Resolution Spectrograph (Sides One and Two) was used to = make ultraviolet spectrographic observations of B3V class standard star = HD210121 (V ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/ftp/observing/status_reports/old_reports_95/hst_status_11_07_95 -- 4.3 Кб -- 07.11.1995
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    75. http://www.stsci.edu/institute/conference/orion/orion-program.doc
    ... 0 | |Turbulence in Molecular Clouds | | | | | |09:30-10:0|Michael Dopita |Superthermal Electrons: The | |0 | ... the Orion Molecular Clouds | | | | | |12:20-12:5|Francisco Salgado |The Orion Nebula in the IR as Seen | |0 | |by SOFIA and Herschel | ...
    [ Текст ]  Ссылки http://www.stsci.edu/institute/conference/orion/orion-program.doc -- 136.5 Кб -- 01.03.2014
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    76. http://www.stsci.edu/ftp/observing/status_reports/old_reports_96/hst_status_12_23_96
    ... 1.20 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 HD28497 whose light passes through a high = galactic molecular ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/ftp/observing/status_reports/old_reports_96/hst_status_12_23_96 -- 13.4 Кб -- 23.12.1996
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    77. HST this week: 081
    ... A Snapshot WFC3 IR Survey of Spitzer/Hershel-Identified Protostars in Nearby Molecular Clouds . 14190 . ... the same manner as stars, by gravitational collapse within molecular clouds, but which do not accrete sufficient mass to raise ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/~inr/thisweek1/2016/thisweek081.html -- 19.8 Кб -- 18.03.2016
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    78. HST this week: 341
    ... A Snapshot WFC3 IR Survey of Spitzer/Hershel-Identified Protostars in Nearby Molecular Clouds . 14199 . ... focused on more than 250 sources within the Orion A molecular cloud, the complex that includes the Orion Nebula Cluster ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/~inr/thisweek1/2015/thisweek341.html -- 21.4 Кб -- 15.12.2015
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    79. No cold dust within the supernova remnant Cassiopeia A
    ... and molecular line observations that demonstrate that most of the detected submillimetre emission originates from interstellar dust in a molecular cloud complex located in the line of sight between the Earth and Cas A, and is therefore not associated with ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/~kgordon/papers/2004Natur.432..596K.html -- 4.1 Кб -- 21.01.2016
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    80. Nino Panagia's Home Page
    ... My main scientific interests include supernovae and supernova remnants, diffuse matter in galaxies (HII regions, molecular clouds and star-forming regions, planetary nebulae, and interstellar dust), stellar winds from early type stars, stellar populations ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/~panagia/ -- 14.1 Кб -- 06.08.2015
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