A POWERFUL NUCLEAR STARBURST IN THE SEYFERT-GALAXY MARKARIAN-477 - IMPLICATIONS FOR THE STARBURST-ACTIVE GALACTIC NUCLEUS CONNECTION

There have been many suggestions that starbursts may play an important role in Seyfert galaxies. Recent analyses of the UV, optical, and nea r-IR ''featureless continuum'' (FC) in type 2 Seyfert nuclei have prov ided indirect evidence that the FC may be produced by a compact starbu rst and that this starburst may provide a power source for the pronoun ced far-IR excess in type 2 Seyfert galaxies. In the present paper, we present and discuss Hubble Space Telescope (HST) images and a UV spec trum plus new ground-based near-UV through near-IR spectra of Mrk 477 (=I Zw 92). This object is arguably the most powerful type 2 Seyfert n ucleus in the local universe and thus offers a unique opportunity for detailed investigation of the nature of the FC. The data provide direc t evidence that the observed UV through near-IR continuum in the nucle us of Mrk 477 is dominated by light from a dusty starburst. An HST ima ge of the space-UV continuum shows that it arises in a compact (few hu ndred parsec) region, much smaller than the sizes of previously studie d circumnuclear starbursts in Seyfert galaxies like NGC 1068. In the H ST space-UV spectrum of this region, we detect strong N V lambda 1240 and Si IV lambda 1400 stellar wind lines and other weak photospheric l ines from hot stars. In the optical spectrum we detect a broad emissio n complex around the He II lambda 4686 line that may be produced by an ensemble of about 30,000 Wolf-Rayet stars (WN subtype). In the near-I R spectrum we detect a strong Ca II triplet feature produced by red su pergiants. Detailed comparison of the data with models implies that th e nuclear starburst in Mrk 477 has an age of about 6 Myr, was of short duration (an ''instantaneous'' burst), and has solar or higher metall icity and a bolometric luminosity of similar to(3 x 10(10))-10(11) L.. This nuclear starburst must therefore make a significant contribution to the overall energetics of Mrk 477, even though optical spectropola rimetry demonstrates that a powerful ''hidden'' type 1 Seyfert nucleus is also present. We speculate that the compact starburst is occurring in the outer reaches of the ''obscuring torus'' that hides the type 1 Seyfert nucleus. An observational program that is underway will deter mine whether Mrk 477 is typical of Seyfert 2 nuclei and, thus, whether nuclear starbursts are an important part of the Seyfert phenomenon.