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Other literature type . 2023
License: CC BY
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Conference object . 2023
License: CC BY
Data sources: Datacite
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Conference object . 2023
License: CC BY
Data sources: Datacite
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Morphological Study of GPS Radio Galaxies

Authors: Carlo Stanghellini; Pietro Cassaro; Cristiana Spingola; Alessandra Zanichelli; Miguel Perez-Torres; C. P. O'Dea; S. A. Baum;

Morphological Study of GPS Radio Galaxies

Abstract

GHz Peaked Spectrum (GPS) radio galaxies show a convex spectrum peaking around 1 GHz and a compact symmetric morphology, which is a scaled-down version (even 1000 times smaller) of those seen in the high power extragalactic radio sources. We suggest that GPS radio galaxies consist of a mixed class of objects, with the majority of them containing a rapidly precessing jet, which is unable to escape the inner region of the host galaxy, making them "frustrated" objects.

Keywords

radio continuum: galaxies, galaxies: active, galaxies: jets

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This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
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popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
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influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
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impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
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