Optical Emission in Double Radio Galaxy Lobes: Cycle 4

Details Optical Emission in Double Radio Galaxy Lobes: Cycle 4 Optical Emission in Double Radio Galaxy Lobes: Cycle 4

Jul 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994hst..prop.5156c&link_type=abstract

HST Proposal ID #5156

Computer Science

Hst Proposal Id #5156 Quasars &Amp, Agn Gas

Scientific paper

Radio hot spots associated with radio galaxies will be studied either to learn about the detailed optical morphology of optical emission already found in the vicinity of the radio emission or to search for new regions where optical emission can be seen. The observations proposed here are of double radio galaxies with compact unresolved components (at 3C resolution). Objects with known emission will be searched using the PC.

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