Uv Studies of Galaxies - Cycle 2

Details Uv Studies of Galaxies - Cycle 2 Uv Studies of Galaxies - Cycle 2

Jul 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992hst..prop.4071d&link_type=abstract

HST Proposal ID #4071

Computer Science

Hst Proposal Id #4071

Scientific paper

The complex nuclear regions of a few typical galaxies will be investigated in order to get the structure both in the continuum and in the light of relevant emission lines with the highest possible resolution. The following objects have been selected. NGC 1365 is a case of active nuclear region in a barred spiral galaxy, which contains optical hot spots and a number of compact radio sources. In NGC 4278, massive hot stars, possibly formed from the gas accumulated in the center, will be searched while mapping the distribution of the ionized gas. NGC 5194 displays in an especially favorable fashion the different manifestations of the energy flow in an active galaxy. The radio elliptical 3C285 exhibits a twisting of isophotes all the way to the center.

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