Results 21 to 30 of about 93,637 (312)

Compact Radio Sources [PDF]

open access: yesSymposium - International Astronomical Union, 1981
SummaryThe observational data on the radio properties of compact radio sources are presented, including their radio spectra, their occurence, and their structures, as well as the variations of the structures in the “superluminal” sources.
K. I. Kellermann, I. I. K. Pauliny-Toth
openaire   +2 more sources

Classical and Relativistic Evolution of an Extra-Galactic Jet with Back-Reaction

open access: yesGalaxies, 2018
We consider a turbulent jet that is moving in a Lane⁻Emden ( n = 5 ) medium. The conserved quantity is the energy flux, which allows finding, to first order, an analytical expression for the velocity and an approximate trajectory.
Lorenzo Zaninetti
doaj   +1 more source

Superluminal Radio Sources [PDF]

open access: yesSymposium - International Astronomical Union, 1988
There are now at least 23 radio sources in which apparent superluminal motion has been found. The effect is not limited to the “classic” examples like 3C 345, but is found in objects with a wide range of characteristic properties. We review the observations of the phenomenon and present an up-to-date list of the known superluminal sources.
Zensus, J. A., Pearson, T. J.
openaire   +3 more sources

The Counts of Radio Sources [PDF]

open access: yesSymposium - International Astronomical Union, 1969
Following the advice of Professor Zel'dovich, I will begin with two platitudes – first, when we consider the implications of the counts of radio sources, we must look at all the counts of radio sources at all frequencies; second, when we attempt to evaluate the implications of the source counts, we should use proper cosmological models and not rely on ...
openaire   +1 more source

A Comprehensive Observational Study of the FRB 121102 Persistent Radio Source

open access: yesThe Astrophysical Journal, 2023
FRB 121102 is the first fast radio burst to be spatially associated with a persistent radio source (QRS 121102), the nature of which remains unknown. We constrain the physical size of QRS 121102 by measuring its flux-density variability with the VLA from
Ge Chen, Vikram Ravi, Gregg W. Hallinan
doaj   +1 more source

An Injection System for the CHIME/FRB Experiment

open access: yesThe Astronomical Journal, 2023
Dedicated surveys searching for fast radio bursts (FRBs) are subject to selection effects that bias the observed population of events. Software injection systems are one method of correcting for these biases by injecting a mock population of synthetic ...
Marcus Merryfield   +21 more
doaj   +1 more source

Extended Radio Sources [PDF]

open access: yesSymposium - International Astronomical Union, 1981
The understanding of the nature of strong radio emission associated with galaxies and quasars has significantly increased in the last five years. A large contribution to this increase has been obtained from the arcsec and milli-arcsec mapping of radio sources which show remarkable features.
openaire   +1 more source

Inferring the Energy and Distance Distributions of Fast Radio Bursts Using the First CHIME/FRB Catalog

open access: yesThe Astrophysical Journal, 2023
Fast radio bursts (FRBs) are brief, energetic, typically extragalactic flashes of radio emission whose progenitors are largely unknown. Although studying the FRB population is essential for understanding how these astrophysical phenomena occur, such ...
Kaitlyn Shin   +20 more
doaj   +1 more source

Temporal and Spectral Properties of the Persistent Radio Source Associated with FRB 20190520B with the VLA

open access: yesThe Astrophysical Journal, 2023
Among more than 800 known fast radio bursts (FRBs), only two, namely FRB 20121102A and FRB 20190520B, are confirmed to be associated with persistent radio sources (PRSs).
Xian Zhang   +14 more
doaj   +1 more source

Extended Radio Emission in the Perhipheral Regions of the Shapley Concentration Core

open access: yesGalaxies, 2017
The Shapley Concentration (SC) is a galaxy supercluster (few tens of degrees) in the Local Universe (<z>∼0.048) which is currently undergoing cluster mergers and group accretion.
Tiziana Venturi   +6 more
doaj   +1 more source

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