ar X iv : a st ro - p h / 99 09 00 7 v 1 1 S ep 1 99 9 Kinematics of ionized and molecular hydrogen in the core of M 100
نویسنده
چکیده
We present high angular and velocity resolution two-dimensional kinematic observations in the spectral lines of Hα and CO J = 1 → 0 of the circumnuclear starburst region in the barred spiral galaxy M100, and compare them with kinematics derived from our previously published numerical modeling. The Hα data, fully sampled and at sub-arcsecond resolution, show a rotation curve that is rapidly rising in the central ∼140 pc, and stays roughly constant, at the main disk value, further out. Non-circular motions are studied from the Hα and CO data by detailed consideration of the velocity fields, residual velocity fields after subtraction of the rotation curve, and sets of position-velocity diagrams. These motions are interpreted as the kinematic signatures of gas streaming along the inner part of the bar, and of density wave streaming motions across a two-armed mini-spiral. Comparison with a two-dimensional velocity field and rotation curve derived from our 1995 dynamical model shows good qualitative and quantitative agreement for the circular and non-circular kinematic components. Both
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تاریخ انتشار 1999