Computer Science
Scientific paper
Jul 2000
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000hst..prop.8665c&link_type=abstract
HST Proposal ID #8665
Computer Science
Hst Proposal Id #8665 Agn/Quasars
Scientific paper
NGC 4303 is to date the best example of the claimed starburst- AGN connection in active galaxies. HST images of NGC 4303 have unveiled the existence of a nuclear mini-bar {250 pc in size}, centered on the unresolved {size <= 8 pc} UV-bright core, itself connected with a star-forming mini-spiral {radius 250 pc}. The spiral consist of compact clusters {size <= 15 pc} of young stars {5-25 Myrs}. The UV-bright core is classified as a Seyfert 2 AGN but its UV luminosity and optical properties are also compatible with the existence of a young { 4 Myr} massive { 10^5 M_odot} cluster of stars. We propose to obtain STIS UV spectra of the unresolved core and the brightest knots in the star-forming mini-spiral of NGC 4303. The spectra will be combined with multifrequency data and evolutionary spectral synthesis models to: {1} pin down the nature of the UV-bright core, i.e. AGN versus young massive stellar cluster, {2} quantify the AGN and starburst energy contribution, {3} determine the age and mass of the star-forming knots, and {4} establish an evolutionary sequence of events within the bar - starburst - AGN scenario. The detection of signatures of massive stars in the spectrum of the core of NGC 4303, would demonstrate for the first time ever that a compact {<= 8 pc} massive stellar cluster is located at the core of a Seyfert 2 galaxy and is, perhaps, its dominant energy source.
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