... of the jet with the cluster gas as a calorimeter (some progress already made! ... the X-ray calorimeter on NeXT, but poor angular resolution - must be used in ...
Mitch Begelman. JILA, University of Colorado. FORMATION AND ... YOU'VE GOT TO BE KIDDING. QUASISTAR PROPERTIES. Mass m* (M ) increases with time. Core with ...
Depends on relative speed but not location of sources. For ... Consider continuously glowing blob, moving almost directly toward you at. 0.8c. 0.8 lt-day ...
How are particles accelerated to relativistic energies? ... Lind et al. 1989. Blandford & Levinson 1995. Sikora, Begelman & Rees 1994. Science: theory ...
Blazars: basic picture. Sikora, Begelman & Rees (1994) Theorists claims that the size of ... Which one's responsible for the X-ray variability? Central engine ...
X-ray Astronomy in the Next Decade. 90% of the matter in the universe can only be ... M.Begelman, TJ Cox, D. Croton, T. DiMatteo, I. George, C. Martin, J. Ostriker, V. ...
... Black hole growth Black hole spin evolution Previous works neglect radiative cooling Radiation is often very important, ... entropy increases inward ...
Yosuke Mizuno ( ) Institute of Astronomy National Tsing-Hua University Collaborators Y. Lyubarsky (Ben-Gurion Univ), K.-I. Nishikawa (NSSTC/UAH), P. E ...
a prominent accretion disk in the low-hard state of the black hole candidate: Truncated disk? There are always OUTLIERS! Accretion Mode in BL Lacs+RLQs (Wang ...
GG Tau: Potter/Hawaii/Gemini/AURA/NSF. 07/11/06. 10. Gas around Binary Black Holes: Alignment ... initial surface density profile. surface density after ...
Fe XXII 11.77 and 11.92 lines give the populations of ... Works for O stars. No. Measure Prad in X-rays. Comparable amount in EUV Fe XXII, XXIII, XXIV ...
A Heino-Centric View of the History of Galactic Center Theory ... Spin, precession and variability of Sgr A*. Linear Polarization images near the event horizon ...
Title: No Slide Title Author: Amir Levinson Last modified by: Admin amir Created Date: 8/26/2002 1:03:38 PM Document presentation format: Pr sentation l' cran (4:3)
I. INTRODUCTION. II. OUR RECENT RESEARCH. III. SUMMARY/CONCLUSION. 3 ... consistent with IMBH mass (iii) Abundance pattern ...consistent with M82 gas, ICM, IGM ...
Agnieszka Janiuk N. Copernicus Astronomical Center, Warsaw Gamma Ray Bursts from Collapsing Massive Stars Collaborations: R. Moderski (CAMK), D. Proga(UNLV), Y. Yuan ...
Advection-Dominated Accretion Flow, ADAF (Ichimaru 1977; Narayan & Yi 1994, 1995; ... We suggest that advection-dominated accretion may provide an explanation for ...
Hot gas dissipates energy through an interface layer into a ... Reflection prevents energy ... May2003Instead, said astronomer Barry Welsh of UC Berkeley's ...
(Rosswog 07; Faber 06; Lee 09) a. r - Process Heating (not included in present simulations! ... NS Matter A ~ 100 Nuclei Free Neutrons (Lattimer 77; Meyer 89) ...
Measurement of halo HI done by comparing Lya absorption against high-Z stars to ... Primordial extragalactic gas, halo supernovae, galactic fountain ...
CLUSTERS OF GALAXIES From Cooling-Flows to Cool Cores X-ray Observatories After the rocket experiments during the 1960s, the first X-ray Earth-orbiting explorers were ...
The thin accretion disk models describes a cooling-dominated flow in which the ... model provides the picture of how gases flow near the vicinity of a black hole ...
D Swartz (MSFC), A Goncalves (Paris-M), R Mushotzky, T ... ULXs may have a persistently. super-Edd accretion rate. High/soft. Very high. ultraluminous ...
Gamma-Ray Burst Early Afterglows. Bing Zhang. Physics Department. University of Nevada, Las Vegas ... gamma-ray. UV/opt/IR/radio. Why is the early afterglow ...
why AGN feedback in Galaxy Clusters? Heating the ICM -- Conduction vs ... Chandra image of Hydra A. For review papers, see. Fabian 1994. Peterson & Fabian 2006 ...
Limb Brightening of the Image a rapid transition an 'overshoot' ... Hydro-simulation: more limb brightening slightly faster transition larger overshoot ...
Radio-to-X-ray diagnostics composition, energy transport, magnetic field geometry ... Example: The Mouse (Gaensler et al. 03) Radio X-ray synchrotron tails ...
Gamma Ray Bursts? 1 ix 05. GLAST GC Meeting. 3. Traditional Disks are: ... X. Can you measure the toroidal field pattern? Even Parity. Odd Parity. Mixed Parity ...
Hot gas dissipates energy through an interface layer into a colder ISM phase. ... cavities and tunnels, analogous to the holes in a sponge, were created ...