Study of Optical Emission Associated with Radio Jets and Hot Spots - Cycle 4

Details Study of Optical Emission Associated with Radio Jets and Hot Spots - Cycle 4 Study of Optical Emission Associated with Radio Jets and Hot Spots - Cycle 4

Jul 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994hst..prop.5144m&link_type=abstract

HST Proposal ID #5144

Mathematics

Logic

Hst Proposal Id #5144 Quasars &Amp, Agn Seyferts

Scientific paper

ST is uniquely equipped to study in detail the narrow line region in nearby AGN. Here we outline a program of broad band imaging on a carefully selected samples of objects designed to exploit ST for these purposes. The aims are to study the following: -structure of the line emission region to test the unified scheme for Seyferts galaxies -morphological relations between radio and optical emission -morphological relations between continuum and line optical emission to detect scattered nuclear emission -ionization state and ionization processes in the NLR from the comparison of different ionization lines, OII and OIII -dynamics of the emitting gas -direct imaging of the ionizing ultraviolet continuum and obscuration properties of the nuclear regions -energetics of the nuclear source compared with observations at other wavelengths, X-ray and IR

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