Studies of Compact Extragalactic Radio Sources

<p>Three studies of compact, extragalactic radio sources are presented.</p> <p>In the first, VLBI maps are presented of the nuclear cores of four radio galaxies which have large symmetric radio lobes: 3C 111, 3C 390.3, Cyg A, and 0055+30. Each source contains a nuclear jet havin...

Full description

Bibliographic Details
Main Author: Linfield, Roger Paul
Format: Others
Language:en
Published: 1981
Online Access:https://thesis.library.caltech.edu/3317/3/linfield_rp_1981.pdf
Linfield, Roger Paul (1981) Studies of Compact Extragalactic Radio Sources. Dissertation (Ph.D.), California Institute of Technology. doi:10.7907/5cg5-0d24. https://resolver.caltech.edu/CaltechETD:etd-09022008-153247 <https://resolver.caltech.edu/CaltechETD:etd-09022008-153247>
id ndltd-CALTECH-oai-thesis.library.caltech.edu-3317
record_format oai_dc
spelling ndltd-CALTECH-oai-thesis.library.caltech.edu-33172021-11-06T05:01:37Z https://thesis.library.caltech.edu/3317/ Studies of Compact Extragalactic Radio Sources Linfield, Roger Paul <p>Three studies of compact, extragalactic radio sources are presented.</p> <p>In the first, VLBI maps are presented of the nuclear cores of four radio galaxies which have large symmetric radio lobes: 3C 111, 3C 390.3, Cyg A, and 0055+30. Each source contains a nuclear jet having a scale of 1 pc, but no counterjets are seen. The jets in 3C 111 and 0055+30 point directly at the outer radio lobes, but in 3C 390.3 and Cyg A the jets are pointed from 4 to 6 degrees away from the lobes.</p> <p>The implications of the maps and models of these sources are considered in the second study. It is concluded that in all four cases, the observed asymmetry reflects an intrinsic asymmetry on a msec scale. The minimum pressure in the four jets is calculated, and it is concluded that the jet in Cyg A is very unlikely to be confined by gas pressure.</p> <p>In the third study, an attempt is made to explain the structure of compact radio sources with a precession-like motion or a relativistic jet. It is found that the curvature of these sources can be readily explained in this way. In addition, the knots which are often revealed by VLBI observations arise naturally in such a model. The main problem with the model is that it cannot by itself explain the arcsecond structure of asymmetric radio sources.</p> 1981 Thesis NonPeerReviewed application/pdf en other https://thesis.library.caltech.edu/3317/3/linfield_rp_1981.pdf Linfield, Roger Paul (1981) Studies of Compact Extragalactic Radio Sources. Dissertation (Ph.D.), California Institute of Technology. doi:10.7907/5cg5-0d24. https://resolver.caltech.edu/CaltechETD:etd-09022008-153247 <https://resolver.caltech.edu/CaltechETD:etd-09022008-153247> https://resolver.caltech.edu/CaltechETD:etd-09022008-153247 CaltechETD:etd-09022008-153247 10.7907/5cg5-0d24
collection NDLTD
language en
format Others
sources NDLTD
description <p>Three studies of compact, extragalactic radio sources are presented.</p> <p>In the first, VLBI maps are presented of the nuclear cores of four radio galaxies which have large symmetric radio lobes: 3C 111, 3C 390.3, Cyg A, and 0055+30. Each source contains a nuclear jet having a scale of 1 pc, but no counterjets are seen. The jets in 3C 111 and 0055+30 point directly at the outer radio lobes, but in 3C 390.3 and Cyg A the jets are pointed from 4 to 6 degrees away from the lobes.</p> <p>The implications of the maps and models of these sources are considered in the second study. It is concluded that in all four cases, the observed asymmetry reflects an intrinsic asymmetry on a msec scale. The minimum pressure in the four jets is calculated, and it is concluded that the jet in Cyg A is very unlikely to be confined by gas pressure.</p> <p>In the third study, an attempt is made to explain the structure of compact radio sources with a precession-like motion or a relativistic jet. It is found that the curvature of these sources can be readily explained in this way. In addition, the knots which are often revealed by VLBI observations arise naturally in such a model. The main problem with the model is that it cannot by itself explain the arcsecond structure of asymmetric radio sources.</p>
author Linfield, Roger Paul
spellingShingle Linfield, Roger Paul
Studies of Compact Extragalactic Radio Sources
author_facet Linfield, Roger Paul
author_sort Linfield, Roger Paul
title Studies of Compact Extragalactic Radio Sources
title_short Studies of Compact Extragalactic Radio Sources
title_full Studies of Compact Extragalactic Radio Sources
title_fullStr Studies of Compact Extragalactic Radio Sources
title_full_unstemmed Studies of Compact Extragalactic Radio Sources
title_sort studies of compact extragalactic radio sources
publishDate 1981
url https://thesis.library.caltech.edu/3317/3/linfield_rp_1981.pdf
Linfield, Roger Paul (1981) Studies of Compact Extragalactic Radio Sources. Dissertation (Ph.D.), California Institute of Technology. doi:10.7907/5cg5-0d24. https://resolver.caltech.edu/CaltechETD:etd-09022008-153247 <https://resolver.caltech.edu/CaltechETD:etd-09022008-153247>
work_keys_str_mv AT linfieldrogerpaul studiesofcompactextragalacticradiosources
_version_ 1719492719990013952