Nfw PowerPoint PPT Presentations

Now, instead of determining the halo profile through calculation, we have a ... Most halo profiles become shallower more gradually than predicted by NFW, NFW ...

T. brucei development in the tsetse fly The fly immune system affects trypanosome ... NFW 1 2 Trypanosoma brucei EP procyclin TsetseEP Trypanosome ...

2) The NFW profile for correctly centered clusters. 3) The NFW convolved with a ... 'Universal' relation from DM sims. Ways of constraining cosmology with clusters ...

Cusp NFW. Soft-Core KING. 2. Constraints to the theories of clusters and ... Verify whether a cusp model (NFW) is prefered over a soft core model (AK) or not ...

of our. Galaxy. Sgr A East SNR ? Black hole ? DM Annihilation ? PWN. Sagittarius A. Colors: H.E.S.S. ... Similar to NFW profile. Angular distribution. syst. ...

Disk bulge NFW halo (oblate/prolate/spherical) ... Surface-of-section of halo orbits map out range of orbits ... Streams in a Prolate Halo ...

... NFW profile from Taylor & Babul, 2004, 2005 ... Milky Way Halo simulated by Taylor & Babul (2005) All-sky map of DM gamma ray emission (Baltz 2006) ...

If radial and constant anisotropy: too fastly rising dispersion near the centre, ... the anisotropy has to be tangential. This is why NFW profiles require 0 ...

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J. BULLOCK. A. COORAY. W. MATHEWS UCSC. F. BRIGHENTI BOLOGNA. OUTLINE. INTRODUCTION ... Lower concentration predicted by simulations (e.g. Bullock et al. 2001) ...

Title: Halo de Mat ria Escura e Anisotropia e Raios C smicos Author: meu Cpmputador Document presentation format: On-screen Show Other titles: Times New Roman ...

... skewed to high values for prolate halos and low values for oblate halos ... Oblate halo. a=0.4, b=1.0. Halos averaged over orientation. and axis ratios ...

Search for Dark Matter with GLAST

The importance of studying dark matter halos: 1)in CDM models, all dark matter ... Physical (Internal) Properties of dark matter halos. Contents. Density profiles ...

DISK KINEMATICS. Sufue & Rubin 2001. DISK KINEMATICS. Decomposing luminosity. distribution of Andromeda Galaxy (Tenjes et al. 1994) ...

Title: Slide 1 Author: Fabio Gastaldello Last modified by: Fabio Created Date: 1/12/2005 10:08:20 AM Document presentation format: Presentazione su schermo (4:3)

... Halo and Ultra High Energy Cosmic Rays Anisotropy. Beatriz B. Siffert UFRJ ... I estimate the anisotropy patterns in the arrival directions map that would be ...

Milky Way properties scale with halo mass. Mstar /Mhalo cooled baryon fraction ... Imply (high) 40% of baryons end up as stars. LMC and other satellites ...

On the other hand .... CDM simulations consistently produce halos that are cusped at the center. This has been known since the 1980 s, and has been popularized by ...

It's z-component is the only one different from zero and increases linearly with ... with the conventional cosmic ray spectra (Strong et al. 2004) new s model ...

Q = ?/ v2 3/2 for collisionless particles Q can not increase. ... 3 halos. X same halo. Density profiles with vth (Avila-Reese et al. 2001) ...

Fukushige 97, Moore 98, Moore 99... Zhao, 1996. singular ... good representation of hot plasma density distribution. galaxies / clusters ...

Title: Slide 1 Author: Fabio Gastaldello Last modified by: Fabio Created Date: 1/12/2005 10:08:20 AM Document presentation format: Presentazione su schermo (4:3)

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X X-ray Study of Mass Distribution in Clusters of Galaxies

?dm(r) = ?1h(r) ?2h(r) All physics can be decomposed ... http://www.ctio.noao.edu/~chrism/current/research/C4/dr3. The SDSS-C4 Galaxy Cluster Catalogue ...

Galaxy formation

Luminous and Dark Matter in Nearby Spiral Galaxies

[ See D. Mazin, N. Tonello and M. L pez talks ] September 2004: Start of regular data-taking ... JOSEP FLIX [IFAE] Where is the sky section? ...

Overcoming Great Barriers in Galactic Archaeology ... Anisotropy of stellar and DM halo. Dark matter. halo and stellar. halo exhibit. quite different ...

Current state of simulations - both DM-only and with baryons ... Mass map overlaid on image of A1689. Diego et al. 2004. Strong Weak Lensing ...

Extended velocity dispersion profile of the brightest cluster galaxy (e.g. Kelson et al. 2002) ... Kelson et al. 2002. Constraints on the inner slope with rsc ...

Statistics of strong gravitational lensing. Observational data. Conclusions. Future. Introduction ... In a concordant cosmology, how large is the core radius? ...

If DM is a fermion and coupled to heavy particles ... coupled to light particles (Z' ... Look like SUSY but relationship between the couplings and MF, ...

Formation and structure of dark matter halos in N-body and SPH ... The Partner Group of Max-Planck-Institute for ... Quasar Absorption Line ...

Cosmological Structure Formation A Short Course III. Structure Formation in the Non-Linear Regime Chris Power

Future of structure in CDM cosmology. Spherical collapse, gravitational binding ... Cosmology. Initially matter-dominated: hierarchical growth of structure ...

Search for Gamma Rays from. LKP Dark Matter in the. UED framework ... correlative observations of transient events. Orbit. 565 km, circular. periode ~95 mns ...

Le halo de mati re noire = interface entre cosmologie et physique des galaxies. ... Mod les analytique. Simulations Num riques. Cluster 6 : Simulation AMR ...

Simon White and the Seven Dwarfs

Self gravitating system of collisionless particles with ... 2: substructure abundance. Moore et al. 1999, ApJ, 524, L19. Self-Interacting Dark Matter (SIDM) ...

Bounding Accretion Pressure, Pac. Entropy Profile, K(r) X-ray Cluster Observations ... Smooth Accretion Model (Voit et al 2003) Phenomenological models vary ...

Dark Matter and Galaxy Formation (Section 3: Galaxy Data vs. Simulations) Joel R. Primack ... Creation of halos and the infall of baryonic matter ...

Relaxed halo unrelaxed halo ( Curir Mazzei 99, 01) HOW THE DISK IS REACTING ... infall, the influence of the Dark Matter structure (triaxiality, substructure. ...

propagation (diffusion in Bfield 0.01-1mG) (Sigl,Biermann et al) ... CMB, WIMPS, neutrino, antimatter- universe composition. Experiments: astro surveys ...

As the most recent structures to assemble in a hierarchical ?CDM ... Bullock et al. 2001. X-ray vs. Lensing Concentrations. Lensing. X-ray 1s scatter. Best-fit ...

The parameters like baryon fraction, mass, spin parameter ... like parameters (baryon fraction, mass ...) and small softening. Using 6% baryons (M33) and ...

Radio galaxies in 6dFGS: influence of the supercluster environment ? ... FLASH FLAIR Hydra Shapley (Kaldare et al. 2003) Hydra-Centaurus cat based (UKST) ...

Slow (dM/dt=0.7 Msun/yr) Rapid (dM/dt=7 Msun/yr) Simulating the post-stripping evolution. ... Slow. No (Shioya et al. 2002, 2004). Spectral evolution: e(b) e(a) ...

Kratek opis programa MSC.Nastran for Windows MSC.visualNastran for Windows Predstavlja kompletno re itev Samostalno orodje za analizo (ne zavisi o CAD) Integracija z ...

Prsentation PowerPoint

Detailed HST-NICMOS (F160W) imaging (from CASTLE) ... (Eigenbrod et al. 2006, A&A 451, 747; data from CASTLEs) Going beyond HST resolution: ...

... one-week and two-week car rentals without making period of analysis adjustments ... International events. Breakeven Analysis. Example 9-9. Sensitivity ...

1901 Max Wolf discover Coma cluster ... 1999 XMM-Newton ESO 0.1-15 keV. 2005 Sukuza Japan. X-ray Clusters. Luminonious X-ray radiation ...