R. Chary, Arp102B, Xi'an Oct 06. 6 /12. H2 lines detected but offset ... R. Chary, Arp102B, Xi'an Oct 06. 10 /12. NIR Spectroscopy: Rodriguez-Ardila et al. 2006 ...
Advection-Dominated Accretion Flow, ADAF (Ichimaru 1977; Narayan & Yi 1994, 1995; ... We suggest that advection-dominated accretion may provide an explanation for ...
... Black hole growth Black hole spin evolution Previous works neglect radiative cooling Radiation is often very important, ... entropy increases inward ...
... ambient conditions around BH Feeding the monster Stellar dynamics & star formation in Galactic Nuclei Useful laboratory for other ... Presentation Last ...
Title: Slide 1 Author: marco salvati Last modified by: salvati Document presentation format: On-screen Show (4:3) Other titles: Arial DejaVu LGC Sans Times New Roman ...
Helical Kink Instabilities in Propagating Poynting-Flux-Dominated Jets ... The helical kink (m=1) or screw mode is, by far, the dominant unstable current ...
Global Three-dimensional MHD Simulations of Black Hole Accretion Flows ... We carried out global 3D MHD simulations of radiatively inefficient black hole ...
Title: GRBs: open issues Author: Gabriele Created Date: 4/25/2004 2:16:39 PM Document presentation format: Presentazione su schermo Other titles: Arial Comic Sans MS ...
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 ...
Global MHD Simulations of State Transitions and QPOs in Black Hole Accretion Flows ... Hardness Intensity Diagram. Power Spectrum. Belloni et al.(2006) fig.2 ...
Towards a 3% Geometric Distance to NGC 4258 ... The Big Picture ... X-ray absorbing layer (nH ~ 1023 cm-2) radius = 0.29 pc where disk crosses line ...
The Duty Cycle of Radio Galaxies. in the context of ... UV flux from first generation of stars and quasars ... Radiatively efficient ('quasar mode') Weak jet ...
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 ...
57 FSRQs and 42 BL Lacs. Redshift for all FSRQs and for 30 BL Lacs ... EGRET blazars. Low power slow cooling large gpeak. Big power fast cooling small gpeak ...
... Black Hole Candidates ... Black hole mass may be constrained from X-ray ... Such a massive black holes may not exist in our Galaxy, but not uncommon ...
(1) Models, (2) Descriptions, and (3) Flows ... Global models of thin accretion disk developed ... picture of how gases flow near the vicinity of a black hole ...
Chaired by Jane Ross. Examined results of past member survey ... Betsy Hiser Scholarship Awarded. Laura Biron- to attend Mindfulness Based Nutrition Training ...
Review of High Energy Astrophysics Research in Mainland China Zhang, Shuang Nan Tsinghua Center for Astrophysics (THCA) and Physics Department Tsinghua University ...
Space Telescope Science Institute. and INAF-IRA. Alessandro Capetti INAF Torino Observatory ... THE HUBBLE SPACE TELESCOPE. 1. What is the origin for ...
Detection of the Intrinsic Size of Sagittarius A* with Closure Amplitude Imaging ... Independent of station-based gain errors. Still dependent on baseline ...
Magnetically-Dominated Accretion Flows Around Black Holes (MDAFs) ... But MDAFs can be 10 times larger than magnetospheres discussed generally heretofore ...
The views expressed in this presentation are those of the ... Micronuclei peripheral blood lymphocytes (PBL) & buccal epithelials 26/26 nurses handling CP ...
Hot and Cold Gas Accretion Modes and Feedback Processes in Radio ... Qualitatively good agreement with known facts. 3C 66B (LERG FRI) Croston et al. (2003) ...
Ringing tail - quasi-normal oscillation of BH. for precision test of general relativity ... Change in number of cycles ,assuming almost spherical accretion ...
III Zw 2 (Brunthaler et al. 2005, A&A, 435, 497): 0.6c at 15 GHz, 1.2c at 43 GHz ... Intrinsic bends by only a few degrees. 3C 446. 0528 134. Changes in Direction ...
INPE Advanced Course on Compact Objects Course IV: Accretion Processes in Neutron Stars & Black Holes Ron Remillard Kavli Center for Astrophysics and Space Research
Des Moines. Washington DC. Chicago (1 school) Tribal. Community (1 school) PE4life Only ... Washington, DC (4 schools) Chicago (1 school) Des Moines (4 schools) ...
Thin disks, H/R 0.1, optically thick, emit the ' Big Blue Bump ' Seyfert ... with galaxy bulges, and a fraction of elliptical galaxies (large bulges) are due ...
Accretion Power in Astrophysics Andrew King Theoretical Astrophysics Group, University of Leicester, UK Accreting Black Holes in a Nearby Galaxy (M101) Accreting ...
M31* - The Nearest Extra-Galactic SMBH. Michael Garcia, Smithsonian ... Position of Crane 1992 pt radio source? ( within 0.5'', accurate to 0.15''...) ~1' ...
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 ...
Differential rotation in a post-merger pulsar (Dai et al. 2006) ... Hyperaccretion disks surrounding pulsars could provide an energy source for some ...
Preliminary Results were appeared in Hayashida, 1998(IAU Sympo 188), and Hayashida, ... X-ray Variability of BHs (from SBHC to AGNs) is Similar to Each Other. ...
Emission Models for Radio Jets Circular Polarization. Heino Falcke ... (Bower, Falcke, Backer et al. 1999a,b,c) Sgr A* Radio Emission - A Few Recent Surprises ...
The profile is skewed with an extended red wing due to gravitational redshift, ... Sagittarius A* An unresolved bright continuum at radio wavelengths ...