The Nucleus of Normal and Starburst Galaxies (fos 20): Cycle 0 Observations

Details The Nucleus of Normal and Starburst Galaxies (fos 20): Cycle 0 Observations The Nucleus of Normal and Starburst Galaxies (fos 20): Cycle 0 Observations

Jul 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990hst..prop.1041b&link_type=abstract

HST Proposal ID #1041

Physics

Hst Proposal Id #1041

Scientific paper

Try to understand the energies of normal galactic nuclei. Are the main sources of ionizing radiation nonthermal, or due to a blue stellar population? High spatial resolution of ST is essential to this problem; FOS spectra can distinguish between a population of hot young stars or HB stars. Use the 0.3" aperture at any central point sources and off nucleus at the appropriate spot determined from WFPC data. Choose this spot within 1", along the major axis in accord with the techniques of FOS program 24, "Dynamics near Cores of Normal Galaxies."

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