Bar pattern speeds in CALIFA galaxies. I. Fast bars across the Hubble sequence
Context. The bar pattern speed (Ωb) is defined as the rotational frequency of the bar, and it determines the bar dynamics. Several methods have been proposed for measuring Ωb. The non-parametric method proposed by Tremaine & Weinberg (1984, ApJ, 282, L5; TW) and based on stellar kinematics is the most accurate. This method has been applied so far
Aguerri, J. A. L. et al.
Fecha de publicación:
4
2015