Low Surface Brighness galaxies: Vc-s0 relation and halo central density radial profile from stellar kinematics measurements

Sissa Medialab Srl (2004) 046

Authors:

Alessandro Pizzella, EM Corsini, E Dalla-Bonta', L Coccato, F Bertola, J Magorrian, M Sarzi

The Cosmological Context of Extraplanar Gas

ArXiv astro-ph/0409639 (2004)

Abstract:

I review evidence that galaxies form from gas that falls into potential wells cold, rather than from virialized gas, and that formation stops once an atmosphere of trapped virialized gas has accumulated. Disk galaxies do not have such atmospheres, so their formation is ongoing. During galaxy formation feedback is an efficient process, and the nuclear regions of disk galaxies blow winds. The cold infalling gas that drives continued star formation has a significant component of angular momentum perpendicular to that of the disk. Extraplanar gas has to be understood in the context set by nuclear outflows and cold skew-rotating cosmic infall.

Can Virialization Shocks be Detected Around Galaxy Clusters Through the Sunyaev-Zel'dovich Effect?

(2004)

Authors:

Bence Kocsis, Zoltan Haiman, Zsolt Frei

Evolution of self-gravitating magnetized disks. II- Interaction between MHD turbulence and gravitational instabilities

(2004)

Authors:

Sebastien Fromang, Steven A Balbus, Caroline Terquem, Jean-Pierre De Villiers

Mapping stationary axisymmetric phase-space distribution functions by orbit libraries

Monthly Notices of the Royal Astronomical Society 353:2 (2004) 391-404

Authors:

J Thomas, RP Saglia, R Bender, D Thomas, K Gebhardt, J Magorrian, D Richstone

Abstract:

This is the first of a series of papers dedicated to unveiling the mass composition and dynamical structure of a sample of flattened early-type galaxies in the Coma cluster. We describe our modifications to the Schwarzschild code of Richstone et al. Applying a Voronoi tessellation in the surface of section, we are able to assign accurate phase-space volumes to individual orbits and to reconstruct the full three-integral phase-space distribution function (DF) of any axisymmetric orbit library. Two types of tests have been performed to check the accuracy with which DFs can be represented by appropriate orbit libraries. First, by mapping DFs of spherical γ-models and flattened Plummer models onto the library, we show that the resulting line-of-sight velocity distributions and internal velocity moments of the library match those derived directly from the DF to a precision better than that of present-day observational errors. Secondly, by fitting libraries to the projected kinematics of the same DFs, we show that the DF reconstructed from the fitted library matches the input DF to a rms of about 15 per cent over a region in phase space covering 90 per cent of the mass of the library. The accuracy achieved allows us to implement effective entropy-based regularization to fit real, noisy and spatially incomplete data.