Title: Slide 1 Last modified by: SCIPP Document presentation format: Custom Other titles: Times New Roman Tahoma Arial Wingdings Avant Garde Gothic Comic Sans MS ...
Hot Cold Molecules: Collisions at Astrophysical Temperatures Frank C. De Lucia Ohio State University * * * * * * * * * * * * * * * * * * Atom Envy, Molecule Envy ...
Spectral modeling and diagnostics in various astrophysical environments Jelle Kaastra SRON Topics Multi-temperature structure Resonance scattering in groups of ...
Vorticity: swirling motions within a flow as. a dynamical entity: long-lived structures ... Interpretation of the vorticity equation. Vortex. stretching ...
a dynamical entity: long-lived structures. due to Kelvin's ... Global Eastward Circulation! More extreme example: Jupiter's cloud bands. Great Red Spot ...
... statistic (Drasco et al. 2003), Probability Event Horizon (Coward et al. 2005) ... Neutron star formation: Blair & Ju 1996, Coward et al. 2001-02, Howell et al. ...
Cosmic Microwave Background Radiation (after-glow from the ... Homogeneity implies isotropy, But isotropy does NOT imply homogeneity. Kepler's laws of motion ...
Double Imaging Spectrograph. Simultaneous red and blue spectra. 3600 to 8000 0.8 to 3 /pixel. GrIm II infrared imager and spectrograph. 1 m to 2.5 m ...
Overview of CMSO Center for Magnetic Self-Organization in Laboratory and Astrophysical Plasmas S. Prager May, 2006 Outline Physics topics Participants Physics goals ...
Very close to the EGRET upper limit for a cluster @ 100Mpc. Many positional coincidence between clusters and un-ID EGRET sources (e.g. Reimer et al. 2003) ...
Numerical simulations of astrophysical plasmas : status and perspectives of the Saclay/DAPNIA software project E. Audit, D. Pomar de, R. Teyssier, B. Thooris
Title: An Updated Library of Reaction Rates for the Astrophysical rp- Process. The importance of Nuclear Structure Effects. Author: sakharuk Last modified by
I will choose as many different scenarios as there are groups. ... X Ray, Gamma Ray and Gravitational Wave Backgrounds. Dark Matter Density and Distribution ...
Understanding the physics of accretion-ejection flows. is central to the understanding of ... Jet acceleration and collimation. Emission from shocks in YSO jets ...
Full theory, including coating anisotropy, different mechanical properties of ... Another approximation: Neglect anisotropy in coating, different parameters ...
The theory implies magnetically-dominated flow in the vicinity of pulsar, as the ... of ideal axisymmetric magneto-hydrodynamics it is possible to accelerate ...
Instituto Nacional de Astrof sica, ptica y Electr nica. Tonantzintla, Puebla, M xico ... Early Universe / Cosmic-rays / astrophysical neutrinos / non baryonic ...
Searching for Astrophysical Neutrinos in Coincidence with Gamma ... source of the highest energy CRs. Produce pions in photomeson reactions with fireball g-rays ...
... the scene includes two isosurfaces, one image and one streamline objects. ... data is displayed and can be used to set interactively the desired contour value. ...
... in 2D dissipation rate. after saturation is sensitive to numerical dissipation: Code Test ... Numerical dissipation is ~1.5 times smaller with. CTU & 3rd ...
New insights on the physics beyond the Standard Model from ... http://meetings.aps.org/link/BAPS.2005.APR.T12.7; Proceedings of the2006Joint APS/JPSMeeting, ...
To accelerate a particle efficiently it must cross the shocks ... Observational panorama: composition. Arrival directions & clustering. H.E.S.S.. 17 h data ...
The acceleration and collimation mechanisms of astrophysical jets are still not ... One of the most promising model for jet launching and collimation is the MHD model. ...
TERWAGNE Guy (LARN FUNDP Namur) ROSS Guy (University of Quebec INRS Varennes) ... Source : V. Quillet et al., Nucl. Instr. Meth. B83 (1993) 47. 14. LARN ...
A low temperature plasma containing disperse particles of solid material, ... If dust particles are charged, they interact with the waves, and give rise ...
Infrared Spectroscopy of Astrophysical Gas, Grains, and Ices with Sofia R. D. Gehrza and E. E. Becklinb aUniversity of Minnesota bUniversities Space Research Association
Astrophysical Exotica: degenerate stars with ultrahigh magnetic fields (white ... Pmag=3x1027 dynes/cm (1022 times larger than Pgas in solar photosphere) ...
Aug/03 Treasury Board approval of submitted budget ($C 20M over ... 16384 spectral channels at widest bandwidth over the 16 GHz. Targetable sub-band feature: ...
Necessity of reverse kinematics. Necessity of absence of deuterium. Characteristics of H standard ... Necessity of absence of deuterium. 1H target. 2D target. q ...
(happy astronomer) The Era of Sky Surveys. Paradigm shift in astronomy: Sky ... With N tropy, you can develop a tree-based algorithm in less time than it would ...
OF STATE, MATTER DENSITY, DARK MATTER. Feb. 18 (NOTE: CLASS ... Dark Matter Density and Distribution. Dark Energy Density and Distribution. Neutrino Background ...
AGB Stars and the s-process. He rich intershell main site for s-process ... normalization done with 6Li(p,p), since targets were prepared under vacuum ...
Brussels, December 2005 ... Volkov (V2) (describes binding energies of triton and 4He) ... data but also the essential properties of the deuteron, triton and 4He) ...