The Jet-Ism Interaction in NGC 5128

Details The Jet-Ism Interaction in NGC 5128 The Jet-Ism Interaction in NGC 5128

Jul 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996hst..prop.6869t&link_type=abstract

HST Proposal ID #6869

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Hst Proposal Id #6869 Stellar Populations

Scientific paper

The radio galaxy NGC 5128 has many peculiarities, one of which is a collection of blue knots and HII regions associated with the eastern side of the northern radio lobe. Spectroscopic studies suggest these objects are complexes of young stars which have been produced under extremely unusual conditions. The objective of the current program is to obtain an optical color-magnitude diagram for these young stellar systems as a means to obtain ages and other stellar population information. We will expose for 3 orbits total in the F450W and F814W filters.

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