Add to ORKGI review our understanding of radio galaxies focusing on their high energy emission properties. Topics addressed include the FR I/II dichotomy, AGN unification, particle acceleration, and the origin of VHE gamma-rays and UHE cosmic ray
We review current understanding of the population of radio galaxies and radio-loud quasars from an o...
This book is a concise primer on galactic radio astronomy for undergraduate and graduate students, a...
Galaxies are filled with particles traveling very close to the speed of light; these are so-called u...
Here in this lecture we will touch on two aspects, one the new radio methods to observe the effects ...
Radio Galaxies have by now emerged as a new γ-ray emitting source class on the extragalactic sk...
During the last decades, various classes of radio-loud active galactic nuclei have been established ...
High-energy gamma-ray astronomy is a field under very rapid development, addressing issues of astrop...
A new class of low-power compact radio sources with limited jet structures, named FR 0, is emerging ...
A brief summary of some highlights in the study of high energy astrophysical sources over the past d...
In this chapter I give an overview of shock acceleration, including a discussion of the maximum ener...
Gamma-ray astronomy which includes the spectral region from above approximately 100 keV to greater t...
We discuss the relation between cosmic-ray induced interstellar gamma-ray and radio emission from ou...
Cross-population radio galaxies (FRII-LERG, i.e., powerful radio sources with an inefficient engine)...
Recently two cosmic rays with energy in excess of 2 1020 eV have been recorded. These are some 108 t...
Ultra high energy cosmic ray events presently show a spectrum, which we interpret here as galactic c...
We review current understanding of the population of radio galaxies and radio-loud quasars from an o...
This book is a concise primer on galactic radio astronomy for undergraduate and graduate students, a...
Galaxies are filled with particles traveling very close to the speed of light; these are so-called u...
Here in this lecture we will touch on two aspects, one the new radio methods to observe the effects ...
Radio Galaxies have by now emerged as a new γ-ray emitting source class on the extragalactic sk...
During the last decades, various classes of radio-loud active galactic nuclei have been established ...
High-energy gamma-ray astronomy is a field under very rapid development, addressing issues of astrop...
A new class of low-power compact radio sources with limited jet structures, named FR 0, is emerging ...
A brief summary of some highlights in the study of high energy astrophysical sources over the past d...
In this chapter I give an overview of shock acceleration, including a discussion of the maximum ener...
Gamma-ray astronomy which includes the spectral region from above approximately 100 keV to greater t...
We discuss the relation between cosmic-ray induced interstellar gamma-ray and radio emission from ou...
Cross-population radio galaxies (FRII-LERG, i.e., powerful radio sources with an inefficient engine)...
Recently two cosmic rays with energy in excess of 2 1020 eV have been recorded. These are some 108 t...
Ultra high energy cosmic ray events presently show a spectrum, which we interpret here as galactic c...
We review current understanding of the population of radio galaxies and radio-loud quasars from an o...
This book is a concise primer on galactic radio astronomy for undergraduate and graduate students, a...
Galaxies are filled with particles traveling very close to the speed of light; these are so-called u...