Deficiency of ``Thin'' Stellar Bars in Seyfert Host Galaxies
Using all available major samples of Seyfert galaxies and their corresponding closely matched control samples of nonactive galaxies, we find that the bar ellipticities (or axial ratios) in Seyfert galaxies are systematically different from those in nonactive galaxies. Overall, there is a deficiency of bars with large ellipticities (i.e., ``thin''
Shlosman, Isaac et al.
Fecha de publicación:
6
2000