paper

Why Are Rotating Elliptical Galaxies Less Elliptical at X-ray Frequencies?

arXiv:astro-ph/0003470 · doi:10.1086/309266

Abstract

If mass and angular momentum were conserved in cooling flows associated with luminous, slowly rotating elliptical galaxies, the inflowing hot gas would spin up, resulting in disks of cold gas and X-ray images that are highly flattened along the equatorial plane out to several effective radii. Such X-ray flattening is not observed at the spatial resolution currently available to X-ray observations. Evidently mass and angular momentum are not in fact conserved. If cooling flows are depleted by localized radiative cooling at numerous sites distributed throughout the flows, then disks of cooled gas do not form and the X-ray images appear nearly circular. However, the distribution of young stars formed from the cooled gas is still somewhat flattened relative to the stellar light. X-ray images of galactic cooling flows can also be circularized by the turbulent diffusion of angular momentum away from the axis of rotation, but the effective viscosity of known processes -- stellar mass loss, supernovae, cooling site evolution, etc. -- is insufficient to appreciably circularize the X-ray images. Radial gradients in the interstellar iron abundance are unaffected by the expected level of interstellar turbulence since these gradients are continuously re-established by Type Ia supernovae.

17 pages with 6 figures; accepted by Astrophysical Journal

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