What are ultraluminous X-ray sources? Tim Roberts.
RevModPhys.76.1143
Tadayuki Takahashi Institute of Space and Astronautical Science (ISAS) Spectral and Temporal Variations of Blazars Hidetoshi Kubo(Kyoto), Jun Kataoka (Tokyo.
The Accretion Mode - Morphology Link in Radio-Loud AGN jets: Towards a More Complete Unification Scheme Eileen Meyer Rice University University of Maryland,
Key points: Active Galactic Nuclei: powerful energy sources in “nuclei” (very center) of some galaxies Main types: Seyferts, radio galaxies and quasars.
March 9, 2011 Special Relativity, continued. Lorentz Transformation Transformation of angles, From formulae for transform Of velocities:
Parsec-scale Jets in Lobe-dominated Quasars David Hough Trinity University Abstract: In order to test relativistic jet and AGN models over a wide range.
Astronomy 1020-H Stellar Astronomy Spring_2015 Day-39.
Key points:
Orbital Characteristics of Extra-Solar Planets
Parsec-scale Jets in Lobe-dominated Quasars David Hough Trinity University
Radio Cores: Particle Accelerators and High-Energy Laboratories VLBI: Krichbaum et al. (1999) Courtesy Heino Falcke TeV neutrinos 511 keV annihilation.
