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Galaxy Interactions and the Radio Galaxy Phenomenon

1990
We have been studying powerful radio galaxies (which we define as having radio power at 178MHz, P 178 ≥ 5xl024 Watts/Hz for a cosmology of H o = 100 km sec-1 Mpc-1 and q o = 0) in order to determine their origins. There are two distinct classes of powerful radio galaxies (PRGs), the so called class A and B radio galaxies (Hine and Longair 1979; Heckman
T. M. Heckman, E. P. Smith
openaire   +2 more sources

A population of red candidate massive galaxies ~600 Myr after the Big Bang

Nature, 2023
Ivo Labbe   +2 more
exaly  

The physics of fast radio bursts

Reviews of Modern Physics, 2023
B-B Zhang
exaly  

Aligned Radio Galaxies

1991
The discovery of high redshift radio galaxies at z ≤ 4 has unleashed a host of questions about their nature. Many new objects are being found, and their unusual properties are being uncovered. They generally exhibit the “alignment effect”, wherein their highly elongated lumpy morphologies are lined up along the axes of their powerful radio sources ...
openaire   +2 more sources

Normal, dust-obscured galaxies in the epoch of reionization

Nature, 2021
Yoshinobu Fudamoto   +2 more
exaly  

The Radio Galaxy

Scientific American, 1959
openaire   +2 more sources

Cool outflows in galaxies and their implications

Astronomy and Astrophysics Review, 2020
Sylvain Veilleux, Roberto Maiolino
exaly  

Emerging Nanotechnology and Advanced Materials for Cancer Radiation Therapy

Advanced Materials, 2017
Guosheng Song, Liang Cheng, Kai Yang
exaly  

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