'Jet power' presentation slideshows

Rob Fender (Southampton)

677 views • 51 slides

The Fermi blazars divide

The Fermi blazars divide. Gabriele Ghisellini Osservatorio Astronomico di Brera In collaboration with L. Maraschi and F. Tavecchio. Bright Fermi blazars. >100 with >10 s detection 57 FSRQs and 42 BL Lacs Redshift for all FSRQs and for 30 BL Lacs. FSRQs. TeV.

649 views • 47 slides

Quasar large scale jets: Fast and powerful or weak and slow, but efficient accelerators?

Quasar large scale jets: Fast and powerful or weak and slow, but efficient accelerators?. Markos Georganopoulos 1,2 1 University of Maryland, Baltimore County 2 NASA Goddard Space Flight Center. Talk overview The situation before Chandra

484 views • 40 slides

Radio L oud AGN Unification: Connecting Jets and Accretion

Radio L oud AGN Unification: Connecting Jets and Accretion. Eileen Meyer Space Telescope Science Institute Giovanni Fossati , Rice University Markos Georganopoulos, UMBC Matthew Lister, Purdue University Invited Talk The Innermost Regions of Relativistic Jets

584 views • 32 slides

Fermi rules out EC/CMB as the X-ray emission mechanism for 3C 273

Fermi rules out EC/CMB as the X-ray emission mechanism for 3C 273. Markos Georganopoulos 1,2 Eileen T. Meyer 3 1 University of Maryland, Baltimore County 2 NASA Goddard Space Flight Center 3 Space Telescope Institute. Talk overview Chandra X-ray emission: Synchrotron of Inverse Compton?

401 views • 30 slides

Minimum e Lorentz factor and matter content of jet in blazars

Minimum e Lorentz factor and matter content of jet in blazars. Qingwen Wu Huazhong University of Science and Technology, China Collaborators: S.-J. Kang & L. Chen Krakow-2015/4/24. 1. Why minimum electron Lorentz factor ?. Crucial for jet power estimation and

311 views • 29 slides

903 views • 26 slides

342 views • 26 slides

Feedback Driven by Radio Sources

Brian McNamara. Feedback Driven by Radio Sources. University of Waterloo. Perimeter Institute for Theoretical Physics Harvard-Smithsonian Center for Astrophysics. Baltimore, STScI May, 9 2012. Collaborators: P. Nulsen (CfA), H. Russell, CJ Ma , C. Kirkpatrick (Waterloo)

371 views • 25 slides

Modeling the Power Evolution of Classical Double Radio Galaxies over Cosmological Scales

242 views • 24 slides

Models for non-HBL VHE Gamma-Ray Blazars

365 views • 23 slides

Acceleration and Energy Transport in the AGN jets: from sub-pc to kpc scale

<outline>. - Acceleration site in the universe. - Acceleration [1] : inner jets < sub-pc jet >. Acceleration [2] : outer jets < kpc jet >. K et al , 2001, ApJ, 560, 659 , 2002, MNRAS, 336, 932. - Energy transport along the jet. - Conclusion. , 2003a, A&A, 399, 91.

485 views • 22 slides

UHECRs from Black Hole Jets of Radio Galaxies

UHECRs from Black Hole Jets of Radio Galaxies. Chuck Dermer Naval Research Laboratory, Washington, DC. Soeb Razzaque (NRL), Justin Finke (NRL), and Armen Atoyan (Concordia U., Montreal). New Journal of Physics, 2009. Outline. UHECR Clustering Observations and GZK Horizon

271 views • 17 slides

Radio Jet Disruption in Cooling Cores

Radio Jet Disruption in Cooling Cores. OR, can radio jets solve the cooling core problem? OR, how do cooling cores disrupt radio jets?. What is a cooling core?.

223 views • 12 slides

Accretion and Ejection in Nearby Low Luminosity AGNs

Accretion and Ejection in Nearby Low Luminosity AGNs. Sgr A* --- LLAGNs --- QSOs Qing-wen Wu Korea Astronomy and Space Science Institute Collaborators: Feng Yuan, Xin-Wu Cao, Min-Feng Gu (Shanghai Obs.) Ya-Di Xu (SJTU). Outline. 1. Introduction

230 views • 11 slides

Numerical Simulations of FRI jets

236 views • 11 slides