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    • [ В начало ] Пред. | 7 | 8 | 9 | 10 | 11 | 12 | 13 | 14 | 15 | 16 | След.

    101. HST this week: 225
    ... Abstract . 10840 . Nuria Calvet, University of Michigan . The FUV fluxes of Tauri stars in the Taurus molecular cloud . Abstract . 10864 . ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/~inr/thisweek1/thisweek225.html -- 14.0 Кб -- 25.09.2007
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    102. HST this week: 260
    ... Abstract . 10840 . Nuria Calvet, University of Michigan . The FUV fluxes of Tauri stars in the Taurus molecular cloud . Abstract . 10872 . ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/~inr/thisweek1/thisweek260.html -- 12.0 Кб -- 05.11.2007
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    103. http://www.stsci.edu/ftp/observing/status_reports/old_reports_95/hst_status_09_15_95
    ... Completed GHRS/1 5895 (The Cool Atomic and Molecular Medium in B3) The High Resolution Spectrograph (Side One) was used to make observations of star HD23625 in order to study the foreground cool atomic and molecular medium of a molecular cloud known as B3 ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/ftp/observing/status_reports/old_reports_95/hst_status_09_15_95 -- 4.9 Кб -- 15.09.1995
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    104. http://www.stsci.edu/hst/wfc3/documents/published/WFC3-WhitePaper-2001.pdf
    ... cores of cold, dusty, and dark molecular clouds, why stars form prodigiously in some ... WFC3 will probe deeply into interstellar molecular clouds where stars are born and ...
    [ Текст ]  Ссылки http://www.stsci.edu/hst/wfc3/documents/published/WFC3-WhitePaper-2001.pdf -- 2360.8 Кб -- 30.12.2009
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    105. http://www.stsci.edu/~marel/decadal/sc/332.pdf
    ... as well as farinfrared polarimetry studies of individual molecular clouds should allow for accurate testing of the hypothesis ...
    [ Текст ]  Ссылки http://www.stsci.edu/~marel/decadal/sc/332.pdf -- 703.0 Кб -- 14.04.2009
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    106. http://www.stsci.edu/ftp/observing/status_reports/old_reports_95/hst_status_08_14_95
    ... Completed GHRS/1 5895 (The Cool Atomic and Molecular Medium in B3) The High Resolution Spectrograph (Side One) was used to make observations of star HD22951 in order to study the foreground cool atomic and molecular medium of a molecular cloud known as B3 ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/ftp/observing/status_reports/old_reports_95/hst_status_08_14_95 -- 8.7 Кб -- 14.08.1995
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    107. HST this week: 330
    ... Links . 10840 . Nuria Calvet, University of Michigan . The FUV fluxes of Tauri stars in the Taurus molecular cloud . Abstract . 10852 . ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/~inr/thisweek1/thisweek330.html -- 15.2 Кб -- 23.11.2007
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    108. http://www.stsci.edu/~kgordon/papers/PS_files/upper_sco_ob2.ps.gz
    ... Other studies have dealt with the ae Oph molecular cloud in great detail, but as this cloud is only a small part of the Upper ...
    [ Текст ]  Ссылки http://www.stsci.edu/~kgordon/papers/PS_files/upper_sco_ob2.ps.gz -- 842.6 Кб -- 23.04.2003
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    109. HST this week: 079
    ... 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/thisweek079.html -- 13.9 Кб -- 19.03.2012
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    110. http://www.stsci.edu/stsci/meetings/space_detectors/ircase.htm
    ... 4, when beyond 800 m m. Study of the molecular hydrogen and C + emission of gas clouds in the early Universe and as a function ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/stsci/meetings/space_detectors/ircase.htm -- 36.1 Кб -- 30.08.2001
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