Observable Consequences of Triaxial Halos
نویسندگان
چکیده
منابع مشابه
Galactic Warps in Triaxial Halos
We study the behaviors of galactic disks in triaxial halos both numerically and analytically to see if warps can be excited and sustained in triaxial potentials. We consider the following two scenarios: 1) galactic disks that are initially tilted relative to the equatorial plane of the halo (for a pedagogical purpose), and 2) tilted infall of dark matter relative to the equatorial plane of the ...
متن کاملThe Influence of Triaxial Halos on Collisionless Galactic Disks
We investigate the effect of rotating, triaxial halos on disk galaxies through an extensive set of numerical N -body simulations. Our simulations use a rigid potential field for the halos and bulges and collisionless particles for the disks. The triaxiality and the rotation rate of the halo are varied, as well as the masses of all three galaxy components. We analyze both the bar stability and t...
متن کاملEvolution of galaxies in triaxial halos with figure rotation
Firstly, we demonstrate that unusually large outer HI spiral arms observed in NGC 2915 can form in an extended gas disk embedded in a massive triaxial dark matter halo with slow figure rotation, through the strong gravitational torque of the rotating halo. Secondly, we show that the figure rotation of a triaxial dark matter halo can influence dynamical evolution of disk galaxies by using fully ...
متن کاملDynamical Models for Disk Galaxies with Triaxial Halos
We construct self-consistent dynamical models for disk galaxies with triaxial, cuspy halos. We begin with an equilibrium, axisymmetric, disk-bulge-halo system and apply an artificial acceleration to the halo particles. By design, this acceleration conserves energy and thereby preserving the system’s differential energy distribution even as its phase space distribution function is altered. The h...
متن کاملThe Orbital Evolution Induced by Baryonic Condensation in Triaxial Halos
Using spectral methods, we analyse the orbital structure of dark matter (DM) in N -body simulations in an effort to understand the physical processes that drive the evolution of dark matter halo shapes caused by growing central masses. A longstanding issue is whether the change in the shapes of DM halos is the result of chaotic scattering of the major family of box orbits that serves as the bac...
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ژورنال
عنوان ژورنال: Symposium - International Astronomical Union
سال: 1987
ISSN: 0074-1809
DOI: 10.1017/s0074180900150405