Radio Source Structure Derived from Interplanetary Scintillation

It is possible to derive information concerning the angular structure of radio sources in the range 0″.1−1″ by making systematic observations of their interplanetary scintillation. A survey of sources from the 3C Revised Catalogue has been made at Cambridge at a frequency of 178 MHz and the observat...

Full description

Saved in:
Bibliographic Details
Published in:Monthly notices of the Royal Astronomical Society 1968-02, Vol.138 (4), p.393-406
Main Authors: Little, L. T., Hewish, A.
Format: Article
Language:English
Citations: Items that cite this one
Online Access:Get full text
Tags: Add Tag
No Tags, Be the first to tag this record!
cited_by cdi_FETCH-LOGICAL-c277t-76ae45b75c48d925352adc7c35ab6df44c081ce609241030c5eba09aafb0592c3
cites
container_end_page 406
container_issue 4
container_start_page 393
container_title Monthly notices of the Royal Astronomical Society
container_volume 138
creator Little, L. T.
Hewish, A.
description It is possible to derive information concerning the angular structure of radio sources in the range 0″.1−1″ by making systematic observations of their interplanetary scintillation. A survey of sources from the 3C Revised Catalogue has been made at Cambridge at a frequency of 178 MHz and the observations and analysis of the data from the survey are described. The conclusions relating to the structure of the individual sources are presented and compared with results obtained by other methods where these are available.
doi_str_mv 10.1093/mnras/138.4.393
format article
fullrecord <record><control><sourceid>istex_cross</sourceid><recordid>TN_cdi_crossref_primary_10_1093_mnras_138_4_393</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>ark_67375_HXZ_3MWKT9T3_2</sourcerecordid><originalsourceid>FETCH-LOGICAL-c277t-76ae45b75c48d925352adc7c35ab6df44c081ce609241030c5eba09aafb0592c3</originalsourceid><addsrcrecordid>eNo9kF1LwzAYhYMoOKfX3vYPdHuTNx_NnTI_NpwIbqJ4E9I0hWrXjiQT_fdWJ16dm_McDg8h5xQmFDRON12wcUqxmPAJajwgI4pS5ExLeUhGACjyQlF6TE5ifAMAjkyOyMWjrZo-W_W74Hy2SmHn0i747MqH5sNXWR36Tbbokg_b1nY-2fCVrVzTpaZtbWr67pQc1baN_uwvx-Tp5no9m-fLh9vF7HKZO6ZUypW0notSCceLSjOBgtnKKYfClrKqOXdQUOclaMYpIDjhSwva2roEoZnDMZnud13oYwy-NtvQbIY7hoL5EWB-BZhBgOFmEDAQ-Z5oYvKf_3Ub3o1UqISZv7wavH--W-s1GobfToJfvQ</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype></control><display><type>article</type><title>Radio Source Structure Derived from Interplanetary Scintillation</title><source>Oxford Open</source><source>EZB Electronic Journals Library</source><creator>Little, L. T. ; Hewish, A.</creator><creatorcontrib>Little, L. T. ; Hewish, A.</creatorcontrib><description>It is possible to derive information concerning the angular structure of radio sources in the range 0″.1−1″ by making systematic observations of their interplanetary scintillation. A survey of sources from the 3C Revised Catalogue has been made at Cambridge at a frequency of 178 MHz and the observations and analysis of the data from the survey are described. The conclusions relating to the structure of the individual sources are presented and compared with results obtained by other methods where these are available.</description><identifier>ISSN: 0035-8711</identifier><identifier>EISSN: 1365-2966</identifier><identifier>DOI: 10.1093/mnras/138.4.393</identifier><language>eng</language><publisher>Oxford, UK: Oxford University Press</publisher><ispartof>Monthly notices of the Royal Astronomical Society, 1968-02, Vol.138 (4), p.393-406</ispartof><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c277t-76ae45b75c48d925352adc7c35ab6df44c081ce609241030c5eba09aafb0592c3</citedby></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>314,776,780,27901,27902</link.rule.ids></links><search><creatorcontrib>Little, L. T.</creatorcontrib><creatorcontrib>Hewish, A.</creatorcontrib><title>Radio Source Structure Derived from Interplanetary Scintillation</title><title>Monthly notices of the Royal Astronomical Society</title><description>It is possible to derive information concerning the angular structure of radio sources in the range 0″.1−1″ by making systematic observations of their interplanetary scintillation. A survey of sources from the 3C Revised Catalogue has been made at Cambridge at a frequency of 178 MHz and the observations and analysis of the data from the survey are described. The conclusions relating to the structure of the individual sources are presented and compared with results obtained by other methods where these are available.</description><issn>0035-8711</issn><issn>1365-2966</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>1968</creationdate><recordtype>article</recordtype><recordid>eNo9kF1LwzAYhYMoOKfX3vYPdHuTNx_NnTI_NpwIbqJ4E9I0hWrXjiQT_fdWJ16dm_McDg8h5xQmFDRON12wcUqxmPAJajwgI4pS5ExLeUhGACjyQlF6TE5ifAMAjkyOyMWjrZo-W_W74Hy2SmHn0i747MqH5sNXWR36Tbbokg_b1nY-2fCVrVzTpaZtbWr67pQc1baN_uwvx-Tp5no9m-fLh9vF7HKZO6ZUypW0notSCceLSjOBgtnKKYfClrKqOXdQUOclaMYpIDjhSwva2roEoZnDMZnud13oYwy-NtvQbIY7hoL5EWB-BZhBgOFmEDAQ-Z5oYvKf_3Ub3o1UqISZv7wavH--W-s1GobfToJfvQ</recordid><startdate>19680201</startdate><enddate>19680201</enddate><creator>Little, L. T.</creator><creator>Hewish, A.</creator><general>Oxford University Press</general><scope>BSCLL</scope><scope>AAYXX</scope><scope>CITATION</scope></search><sort><creationdate>19680201</creationdate><title>Radio Source Structure Derived from Interplanetary Scintillation</title><author>Little, L. T. ; Hewish, A.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c277t-76ae45b75c48d925352adc7c35ab6df44c081ce609241030c5eba09aafb0592c3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>1968</creationdate><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Little, L. T.</creatorcontrib><creatorcontrib>Hewish, A.</creatorcontrib><collection>Istex</collection><collection>CrossRef</collection><jtitle>Monthly notices of the Royal Astronomical Society</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Little, L. T.</au><au>Hewish, A.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Radio Source Structure Derived from Interplanetary Scintillation</atitle><jtitle>Monthly notices of the Royal Astronomical Society</jtitle><date>1968-02-01</date><risdate>1968</risdate><volume>138</volume><issue>4</issue><spage>393</spage><epage>406</epage><pages>393-406</pages><issn>0035-8711</issn><eissn>1365-2966</eissn><abstract>It is possible to derive information concerning the angular structure of radio sources in the range 0″.1−1″ by making systematic observations of their interplanetary scintillation. A survey of sources from the 3C Revised Catalogue has been made at Cambridge at a frequency of 178 MHz and the observations and analysis of the data from the survey are described. The conclusions relating to the structure of the individual sources are presented and compared with results obtained by other methods where these are available.</abstract><cop>Oxford, UK</cop><pub>Oxford University Press</pub><doi>10.1093/mnras/138.4.393</doi><tpages>14</tpages><oa>free_for_read</oa></addata></record>
fulltext fulltext
identifier ISSN: 0035-8711
ispartof Monthly notices of the Royal Astronomical Society, 1968-02, Vol.138 (4), p.393-406
issn 0035-8711
1365-2966
language eng
recordid cdi_crossref_primary_10_1093_mnras_138_4_393
source Oxford Open; EZB Electronic Journals Library
title Radio Source Structure Derived from Interplanetary Scintillation
url http://sfxeu10.hosted.exlibrisgroup.com/loughborough?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-01-31T04%3A44%3A03IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-istex_cross&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Radio%20Source%20Structure%20Derived%20from%20Interplanetary%20Scintillation&rft.jtitle=Monthly%20notices%20of%20the%20Royal%20Astronomical%20Society&rft.au=Little,%20L.%20T.&rft.date=1968-02-01&rft.volume=138&rft.issue=4&rft.spage=393&rft.epage=406&rft.pages=393-406&rft.issn=0035-8711&rft.eissn=1365-2966&rft_id=info:doi/10.1093/mnras/138.4.393&rft_dat=%3Cistex_cross%3Eark_67375_HXZ_3MWKT9T3_2%3C/istex_cross%3E%3Cgrp_id%3Ecdi_FETCH-LOGICAL-c277t-76ae45b75c48d925352adc7c35ab6df44c081ce609241030c5eba09aafb0592c3%3C/grp_id%3E%3Coa%3E%3C/oa%3E%3Curl%3E%3C/url%3E&rft_id=info:oai/&rft_id=info:pmid/&rfr_iscdi=true