High-Resolution Surface Photometry of NGC 4314 : Cycle 0

Details High-Resolution Surface Photometry of NGC 4314 : Cycle 0 High-Resolution Surface Photometry of NGC 4314 : Cycle 0

Jul 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990hst..prop.1012j&link_type=abstract

HST Proposal ID #1012

Physics

Hst Proposal Id #1012

Scientific paper

We propose to obtain ST WF/PC surface photometry of NGC 4314. NGC 4314 exhibits anomalous nuclear activity indicative of on-going star formation. Multicolor surface photometry with 0.1 to 0.4 arcsec resolution will afford an opportunity to explore the global interrelationships between gas clouds, dust, star formation, and stellar populations with detail never before obtained. The expected maximum resolution for for NGC 4314 is 10 parsecs. While most of the data will be secured after the refurb mission with WFPC II, these early I-band exposures will allow studies of structures.

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