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Roger Blandford

Researcher at Stanford University

Publications -  716
Citations -  97353

Roger Blandford is an academic researcher from Stanford University. The author has contributed to research in topics: Galaxy & Fermi Gamma-ray Space Telescope. The author has an hindex of 156, co-authored 704 publications receiving 90181 citations. Previous affiliations of Roger Blandford include SLAC National Accelerator Laboratory & Max Planck Society.

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Black hole magnetosphere with small-scale flux tubes - II. Stability and dynamics

TL;DR: In this paper, the authors consider the possibility that this X-ray source may be powered by small scale magnetic flux tubes attached to the accretion disk near the supermassive black hole and study the dynamics of such flux tubes as they get continuously twisted by the central compact star/black hole.
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Suzaku observations of luminous quasars: revealing the nature of high-energy blazar emission in low-level activity states

A. A. Abdo, +210 more
TL;DR: In this paper, the authors presented the results from the Suzaku X-ray observations of five flat-spectrum radio quasars (FSRQs), namely PKS0208-512, Q0827+243, PKS1127-145,PKS1510-089 and 3C 454.3, which revealed the nature of high-energy emission of luminous blazars in their low-activity states.
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Measurements of resonant scattering in the Perseus cluster core with Hitomi SXS

Felix Aharonian, +193 more
TL;DR: In this article, the velocities of gas motions, metallicities and the multi-temperature structure of the gas in the core of the Perseus cluster were measured using the Soft X-ray Spectrometer (SXS) on board Hitomi.
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Strong Redshift Clustering of Distant Galaxies

TL;DR: In this paper, the authors present initial results from a redshift survey carried out with the Low Resolution Imaging Spectrograph on the 10~m W. M. Keck Telescope of a field 14.6 arc-min$^2$ in solid angle.
Journal Article

Evidence for enhanced MHD turbulence outside sharp-rimmed supernova remnants

TL;DR: In this article, the authors consider the propagation of synchrotron-emitting electrons near the shocks of supernova remnants and show that for the sharpest rims, this mean free path is typically less than one percent of that derived for cosmic rays of similar rigidity in the interstellar medium.