The nuclear starburst activity in the Seyfert 2 galaxy NGC 7679
arXiv:astro-ph/0106165 · doi:10.1051/0004-6361:20010806
Abstract
We present our recent spectrophotometric results of the infrared luminous Seyfert 2 galaxy NGC 7679. We find compelling evidence of the presence of a recent nuclear starburst, revealed by the observations of a) the spectral features of high order Balmer absorption lines, b) the weak equivalent widths for CaIIK 3933, CN 4200, G-band 4300 and MgIb 5173, and c) the suggested UV stellar wind resonance lines (N V 1240, Si IV 1400 and C IV 1550) in the IUE spectrum. Using the simple stellar population synthesis model, we find that in the nuclear 2" 2" region, the contributions from the old, intermediate and young components are 21.7%, 42.9% and 35.4%, respectively. These nuclear starburst activities might be triggered by the close encounter with NGC 7682, as suggested by recent numerical simulations.
arXiv comment8 pages, 3 figures, to be published in A&A
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