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Galaxy Interactions and the Radio Galaxy Phenomenon
1990We 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
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A population of red candidate massive galaxies ~600 Myr after the Big Bang
Nature, 2023Ivo Labbe+2 more
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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 ...
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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, 2021Yoshinobu Fudamoto+2 more
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Cool outflows in galaxies and their implications
Astronomy and Astrophysics Review, 2020Sylvain Veilleux, Roberto Maiolino
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Emerging Nanotechnology and Advanced Materials for Cancer Radiation Therapy
Advanced Materials, 2017Guosheng Song, Liang Cheng, Kai Yang
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The dispersion–brightness relation for fast radio bursts from a wide-field survey
Nature, 2018J R Allison, Gülay Gürkan
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