... 1.6 Completed FOS/RD 6505 (Confirming the Quasar in Cygnus-A) The Faint Object Spectrograph (Red Side) was used to make = spectrographic observations of Cygnus-A in order to confirm the presence = of Mg II emission lines. ...
... Seyfert Galaxies) The Faint Object Camera (f/96) was used to make observations at several wavelengths of Seyfert galaxy MRK78 and Cygnus A, to study the narrow line region, the morphology relations between radio and optical emission and continuum and line ...
... 1.5 Completed WF/PC-2 5779 (Miscellaneous - HH7-11 and Cyg Loop - Cycle 4) The WF/PC-2 was used to obtain images of HH7-11 and several regions in the Cygnus Loop. ...
... Seyfert Galaxies) The Faint Object Camera (f/96) was used to make observations at several wavelengths of Seyfert galaxy MRK3 and Cygnus A, to study the narrow line region, the morphology relations between radio and optical emission and continuum and line ...
... 1.5 Completed FOC/96 5140 (Observations of the Narrow Line Regions in Nearby Seyfert Galaxies) The Faint Object Camera (f/96) was used to make observations at several different wavelengths of a Seyfert galaxy which is located near the Cygnus A source. ...
... 1.19 Completed STIS/CCD 9123 (Synchrotron Self-Compton Emission from the Radio Hot Spots of Cygnus A) The Space Telescope Imaging Spectrograph (CCD) was used to observe radio galaxy Cygnus A recently studied in X-rays with Chandra. ...
... 1.7 Completed FOC/96 5140 (Observations of the Narrow Line Regions in Nearby Seyfert Galaxies) The Faint Object Camera (f/96) was used to make observations at several different wavelengths of Seyfert galaxy MRK-6 which is located near the Cygnus A source. ...
... Scheduled for launch in June 2008, Kepler will continuously monitor ~100,000 (mainly) so lar-type stare within a ~100 square degree region in Cygnus. ...
... 9080 (Transition from Non-radiative to Radiative Shocks in the Cygnus Loop) The WF/PC-2 was used to obtain narrow band HAlpha and O III imaging of faint filaments in the northeastern Cygnus Loop that represent the location of the primary shock front as it ...
... Scheduled for launch in June 2008, Kepler will continuously monitor ~100,000 (mainly) so lar-type stare within a ~100 square degree region in Cygnus. ...