Isochrone potential. Some Examples for Spherical Systems. Modified Hubble profile ... Kuzmin's model(1956)(Toomre's model 1) Potential-Density Pairs for ...
Session H1: Local Helioseismology I: Current Issues 3:15-3:30 Turbulent magnetohydrodynamics of the Sun: big questions and key targets for HMI - J.Toomre
Does it work the same way in nature? Mixture of evidence from real data and ... Toomre & Zang introduced central cutout and an outer taper in active density ...
Provide acoustic signature data to test/calibrate inversion methods. Approach ... Anelastic approx. Derive acoustic field. Full-sphere artificial data ...
Gary A Glatzmaier. University of California, Santa Cruz. Direct simulation of ... Glatzmaier, Roberts. Geodynamo model. Anelastic with rbot / rtop = 1.2 ...
Dynamics: Nic Brummell, Sacha Brun, Marc DeRosa, Mark Miesch. Just ... POLEWARD. FLOW NEAR. SURFACE. REVERSED. FLOW. AT DEPTH. 1997. 1996. Haber et al (2002) ...
2. SF laws: KS versus Schmidt ... Sound speed (from velocity dispersion, or not!) Surface density ... Buts: C may depend on density. Kennicutt-Schmidt ...
Session 6 Key Questions for Understanding This Unusual Solar Minimum Alan Gabriel Todd Hoeksema Janet Luhmann Bill Matthaeus Neil Sheeley Key Questions for ...
(vorticity in the axisymmetric flow flield has a local extremum) ... We believe that the origin of the shear instability lies on the vorticity creation on shocks. ...
This shows the heavy element abundance in the four major planets and estimated uncertainties ... Runway growth of core until depletion of heavies in feeding ...
Respond to discussion (Thur) on 'we are made of star stuff, and how does it come ... Correct position relative to new moon for Crab Supernova, but some doubt ...
gravitational torques (Hoyle 49; Peebles 69). High-resolution simulations find no ... Minor mergers don t change. or even decrease (d Onghia & Burkert, astro ...
Helioseismology measures flows below active regions. Relation ... Helioseismology. uses acoustic waves that propagate throughout the Sun to measure the internal ...
M51, the Whirlpool Galaxy. Lord Rosse discovered the spiral structure in M51 in 1850 ... Processes could take place in disk galaxies. Controlling bar instability ...
UN ESTUDIO DE ESCENARIOS INESTABLES EN LA GALAXIA NGC 5427. Vlad mir Jearim PE A-SU REZ, F s. ... Sy II espiral de dos brazos con extensas ... (Combes, 2000) ...
STAR FORMATION RATE E MORFOLOGIA DELLE GALASSIE formazione stellare tecniche osservative correlazioni morfologiche Simone Callegari, Esame di Astronomia ...
dust emission with a scale of 100-400 AU. Outer radius ... Calvet et al. (1994) showed SEDs can be explained by dust emission from an infalling envelope ...
Observations de la Mati re Noire Fran oise Combes Observatoire de Paris (Luminy Septembre 02) Quelques points abord s Courbes de rotation Forme g n rale de tous ...
Rotation is the main cause of mixing in stellar radiation zones. It plays a major role in the ... changes advection of chemicals into vertical diffusion ...
Uses evanescent wave to selectively excite fluorophores within about 100nm of a ... Creating the Evanescent Wave ... Coupling to evanescent modes without a prism. ...
a first approximation, stellar disks in spiral galaxies may be regarded as having a zero ... of the epicycle approximation in spiral galaxies by calculating ...
have rotation rates such that Vrot ~ 0.3-2 x Vrot (Jupiter) after. contraction down to the mean ... Snapshots of sims with different. Tcool, all after ~ 10 Torb ...
Title: Space Weather Magnetic Field Origins Author: Art Poland Last modified by: Art Poland Created Date: 9/15/2005 12:41:40 AM Document presentation format
Lipid Raft and Signal Transduction Tao Chen Lipid Raft A cholesterol-enriched microdomain in cell membrane. A liquid-ordered phase dispersed in a liquid disordered ...
Initial Stages of Planet Formation in Protoplanetary Disks: Origin of Vortices A. G. Tevzadze Abastumani Astrophysical Observatory, Georgia Tbilisi State University ...
Asteroids (carbonaceous chondrites) beyond ice line (2.5 AU) can have high water ... Perturbations by Jupiter of asteroid system perturbs their orbits into ellipses ...
A major puzzle: 'The Mice' NGC 4676 'Mice' with HST Advanced Camera for Surveys ' ... Quasi-Stellar Radio Source (QSO) arise from early galaxy collisions feeding BH? ...
Kuzmin and Stellar Dynamics Introduction Dynamical models G.G. Kuzmin s pioneering work Mass models, orbits, distribution functions Structure of triaxial galaxies
In the optical continuum, NGC 2915 is a nondescript Blue Compact Dwarf galaxy ... 767 (see Fig. 2) was observed with the ANU2.3m telescope DBS spectrograph ...
Title: Presentazione di PowerPoint Author: Pasotti Francesco Last modified by: Guido Chincarini Created Date: 6/27/2005 6:29:45 PM Document presentation format
Molecular gas in Tidal Dwarf Galaxies: Exploring the conditions ... Stephane Leon. Vassilis Charmandaris. Elias Brinks. C. Mundell. P. Appleton. E. Schinnerer ...
3:30-3:40 Time-distance helioseismology of the deep interior - T.L.Duvall, Jr ... the Science Plan and HMI Data Analysis Pipeline from the participants. ...