... UV/Optical Spectroscopy of H-II Regions in the Magellanic Clouds) Both the WF/PC-2 and the Space Telescope Imaging Spectrograph (CCD) were used to make high signal/noise, ultraviolet and optical observations of the H-II region in the Large Magellanic ...
... Sets of STIS/CCD/MA1/MA2 8043 (Physical Properties of H-I and H-II Regions) The Space Telescope Imaging Spectrograph (CCD, MA1 and MA2) was used to make observations of the early-type stars HD210839 and HD94493 in order to study their H-I and H-II regions ...
... 1.5 Completed STIS/CCD/MA1 8043 (Physical Properties of H-I and H-II Regions) The Space Telescope Imaging Spectrograph (CCD and MA1) was used to make observations of the early-type star HD224151 in order to study its H-I and H-II regions. ...
... 1.11 Completed STIS/CCD/MA1 8043 (Physical Properties of H-I and H-II Regions) The Space Telescope Imaging Spectrograph (CCD and MA1) was used to make observations of the early-type star HD106343 in order to study its H-I and H-II regions. ...
... UV/Optical Spectroscopy of H-II Regions in the Magellanic Clouds) Both the WF/PC-2 and the Space Telescope Imaging Spectrograph (CCD) were used to make high signal/noise, ultraviolet and optical observations of the H-II region in the Large Magellanic ...
... 1.11 Completed STIS/CCD/MA1 8043 (Physical Properties of H-I and H-II Regions) The Space Telescope Imaging Spectrograph (CCD and MA1) was to be used to make observations of the early-type star HD3827 in order to study its H-I and H-II regions. ...