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    1. http://www.stsci.edu/ftp/observing/status_reports/old_reports_95/hst_status_12_18_95
    ... 1.5 Completed WF/PC-2 6056 (Spectroscopy and Imagery of the Orion = Nebula) The WF/PC-2 was used to make observations of selected sections of = the Orion Nebula (aka, NGC-1976). ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/ftp/observing/status_reports/old_reports_95/hst_status_12_18_95 -- 8.7 Кб -- 18.12.1995
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    2. An HST Survey of the Inner Regions of the Orion Nebula
    ... attention of the Orion Nebula (M42, NGC 1976) and its associated Trapezium Cluster ... This attention is well deserved because NGC 1976 is the closest bright HII region ... The basic elements of the structure of NGC 1976 are well understood. ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/stsci/meetings/shst2/odellr.html -- 29.2 Кб -- 15.06.2005
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    3. http://www.stsci.edu/ftp/observing/status_reports/old_reports_94/hst_status_09_16_94
    ... observations of the nearby active galactic nuclei of NGC-1976 to study the interactions between the central engine, the stars ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/ftp/observing/status_reports/old_reports_94/hst_status_09_16_94 -- 3.7 Кб -- 16.09.1994
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    4. http://www.stsci.edu/ftp/observing/status_reports/old_reports_95/hst_status_11_15_95
    ... WF/PC-2 was used to make observations of star cluster NGC-1976 = which is known to be one of the oldest clusters in the Large ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/ftp/observing/status_reports/old_reports_95/hst_status_11_15_95 -- 6.5 Кб -- 15.11.1995
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    5. http://www.stsci.edu/ftp/observing/status_reports/old_reports_99/hst_status_02_03_99
    ... Disks in the Orion Nebula) The Space Telescope Imaging Spectrograph (CCD) and the WF/PC-2 were used to make multi-wavelength imaging of circumstellar disks (NGC-1976) seen as silhouettes against the bright emission-line background in the Orion Nebula ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/ftp/observing/status_reports/old_reports_99/hst_status_02_03_99 -- 8.2 Кб -- 03.02.1999
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    6. http://www.stsci.edu/ftp/observing/status_reports/old_reports_95/hst_status_02_06_95
    ... 1.5 Completed WF/PC-2 5085 (Turbulence in H II Regions) The WF/PC-2 was used to make observations of the small scale turbulent H II regions located in NGC-1976-8 (aka, the Orion Nebula) using several different line and continuum filters. ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/ftp/observing/status_reports/old_reports_95/hst_status_02_06_95 -- 10.7 Кб -- 06.02.1995
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    7. http://www.stsci.edu/ftp/observing/status_reports/old_reports_95/hst_status_10_16_95
    ... 1.14 Completed GHRS/2 6056 (Spectroscopy and Imagery of the Orion = Nebula) The High Resolution Spectrograph (Side Two) was used to make = observations of selected sections of the Orion Nebula (aka, NGC-1976). ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/ftp/observing/status_reports/old_reports_95/hst_status_10_16_95 -- 11.1 Кб -- 16.10.1995
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    8. http://www.stsci.edu/ftp/observing/status_reports/old_reports_98/hst_status_02_23_98
    ... Disks in the Orion Nebula) The Space Telescope Imaging Spectrograph (CCD) and the WF/PC-2 was used to make multi-wavelength imaging of circumstellar disks (NGC-1976) seen as silhouettes against the bright emission-line background in the Orion Nebula ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/ftp/observing/status_reports/old_reports_98/hst_status_02_23_98 -- 15.2 Кб -- 23.02.1998
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    9. http://www.stsci.edu/ftp/observing/status_reports/old_reports_95/hst_status_01_03_95
    ... 1.23 Completed WF/PC-2 5085 (Turbulence in H II Regions) The WF/PC-2 was used to make observations of the small scale turbulent H II regions located in NGC-1976-9 (aka, the Orion Nebula) using several different line and continuum filters. ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/ftp/observing/status_reports/old_reports_95/hst_status_01_03_95 -- 11.6 Кб -- 03.01.1995
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    10. http://www.stsci.edu/ftp/observing/status_reports/old_reports_99/hst_status_09_22_99
    ... Determination of Circumstellar Cloud Mass Loss Rates with STIS Spectra) Both the WF/PC-2 and the Space Telescope Imaging Spectrograph (MA2) were used to make observations of the star cluster NGC-1976 to determine its circumstellar cloud mass loss rate ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/ftp/observing/status_reports/old_reports_99/hst_status_09_22_99 -- 9.0 Кб -- 22.09.1999
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