Young Populations in the Nuclei of Barred Galaxies |
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Authors: | HB Ann |
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Institution: | (1) Dept. of Earth Science, Pusan National University, South Korea E-mail |
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Abstract: | We have conducted UBVRI and Hα CCD photometry of five barred galaxies (NGC 2523, NGC 2950, NGC 3412, NGC 3945 and NGC 5383),along with SPH simulations,
in order to understand the origin of young stellar populations in the nuclei of barred galaxies. The Hα emission, which is thought to be emitted by young stellar populations, is either absent or strongly concentrated in the nuclei
of early-type galaxies (NGC 2950, NGC 3412 and NGC 3945),while they are observed in the nuclei and circumnuclear regions of
intermediate-type galaxies with strong bars (NGC 2523 and NGC 5383).SPH simulations of realistic mass models for these galaxies
show that some disc material can be driven into the nuclear region by a strong bar potential. This implies that the young
stellar populations in the circumnuclear regions of barred galaxies can be formed out of such gas. The existence of nuclear
dust lanes is an indication of an ongoing gas inflow and extremely young stellar populations in these galaxies, because nuclear
dust lanes such as those in NGC 5383 are not long-lasting features according to our simulations.
This revised version was published online in July 2006 with corrections to the Cover Date. |
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