The blazar 0059+581: Successful prognosis of activity

Our earlier joint analysis of light curves for the blazar 0059+581 at 4.8, 8, 14.5, 22, and 37 GHz with high-resolution VLBI images led us to suggest that the activity in this source develops in cycles, or periods, with a duration of about four years, with a 'typical scenario' for the deve...

Full description

Saved in:
Bibliographic Details
Published in:Astronomy reports 2006-06, Vol.50 (6), p.468-482
Main Authors: Pyatunina, T B, Gabuzda, D C, Jorstad, S G, Kudryavtseva, N A, Aller, M F, Aller, H D, Terasranta, H
Format: Article
Language:English
Subjects:
Astronomy
Astrophysics
Quasars
Radio astronomy
Citations: Items that this one cites
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-c367t-40a48b1039541fd549607a7baca384995b8c7ea752c520cdd3cb36433da8435c3
cites cdi_FETCH-LOGICAL-c367t-40a48b1039541fd549607a7baca384995b8c7ea752c520cdd3cb36433da8435c3
container_end_page 482
container_issue 6
container_start_page 468
container_title Astronomy reports
container_volume 50
creator Pyatunina, T B
Gabuzda, D C
Jorstad, S G
Kudryavtseva, N A
Aller, M F
Aller, H D
Terasranta, H
description Our earlier joint analysis of light curves for the blazar 0059+581 at 4.8, 8, 14.5, 22, and 37 GHz with high-resolution VLBI images led us to suggest that the activity in this source develops in cycles, or periods, with a duration of about four years, with a 'typical scenario' for the development of the source's activity taking place over a cycle. Based on this analysis, we predicted in 2002 that a new superluminal component would be ejected from the core of this source in a structural position angle ~170DG no later than by the end of 2003. A 43-GHz VLBI image obtained on September 14, 2003, as part of a program to monitor the structure of reference sources used for a radio astronomical coordinate system, convincingly confirms the correctness of this prediction. This is the first time in the history of radio astronomy that a new superluminal component has been detected at a predicted time and in a predicted structural position angle.
doi_str_mv 10.1134/S1063772906060060
format article
fullrecord <record><control><sourceid>proquest_cross</sourceid><recordid>TN_cdi_proquest_miscellaneous_902347948</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>743629284</sourcerecordid><originalsourceid>FETCH-LOGICAL-c367t-40a48b1039541fd549607a7baca384995b8c7ea752c520cdd3cb36433da8435c3</originalsourceid><addsrcrecordid>eNqFkU1LA0EMhgdRsFZ_gLfFgx5kNTOZT29S_IKCh9bzMjs7q1u23TqzK9Rf75R6UtAkkEAe3iSEkFMKV5Qiv55RkKgUMyCTp9gjIyoky6XWdD_VqZ1v-4fkKMYFAKUa5YiI-ZvPytZ-2pABCHMpNL3JZoNzPsZ6aLN16F5XXWxi1tWZdX3z0fSbY3JQ2zb6k-88Ji_3d_PJYz59fnia3E5zh1L1OQfLdUkBjeC0rgQ3EpRVpXUWNTdGlNopb5VgTjBwVYWuRMkRK6s5CodjcrHTTVu8Dz72xbKJzretXfluiIUBhlwZrv8lFUfJDEuyY3L-J8mA8WSQwLMf4KIbwirdWyhhNGNabOfSHeRCF2PwdbEOzdKGTUGh2H6m-PUZ_AKtM3wx</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>759822858</pqid></control><display><type>article</type><title>The blazar 0059+581: Successful prognosis of activity</title><source>Springer Link</source><creator>Pyatunina, T B ; Gabuzda, D C ; Jorstad, S G ; Kudryavtseva, N A ; Aller, M F ; Aller, H D ; Terasranta, H</creator><creatorcontrib>Pyatunina, T B ; Gabuzda, D C ; Jorstad, S G ; Kudryavtseva, N A ; Aller, M F ; Aller, H D ; Terasranta, H</creatorcontrib><description>Our earlier joint analysis of light curves for the blazar 0059+581 at 4.8, 8, 14.5, 22, and 37 GHz with high-resolution VLBI images led us to suggest that the activity in this source develops in cycles, or periods, with a duration of about four years, with a 'typical scenario' for the development of the source's activity taking place over a cycle. Based on this analysis, we predicted in 2002 that a new superluminal component would be ejected from the core of this source in a structural position angle ~170DG no later than by the end of 2003. A 43-GHz VLBI image obtained on September 14, 2003, as part of a program to monitor the structure of reference sources used for a radio astronomical coordinate system, convincingly confirms the correctness of this prediction. This is the first time in the history of radio astronomy that a new superluminal component has been detected at a predicted time and in a predicted structural position angle.</description><identifier>ISSN: 1063-7729</identifier><identifier>EISSN: 1562-6881</identifier><identifier>DOI: 10.1134/S1063772906060060</identifier><language>eng</language><publisher>Heidelberg: Springer Nature B.V</publisher><subject>Astronomy ; Astrophysics ; Quasars ; Radio astronomy</subject><ispartof>Astronomy reports, 2006-06, Vol.50 (6), p.468-482</ispartof><rights>Nauka/Interperiodica 2006</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c367t-40a48b1039541fd549607a7baca384995b8c7ea752c520cdd3cb36433da8435c3</citedby><cites>FETCH-LOGICAL-c367t-40a48b1039541fd549607a7baca384995b8c7ea752c520cdd3cb36433da8435c3</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>314,780,784,27924,27925</link.rule.ids></links><search><creatorcontrib>Pyatunina, T B</creatorcontrib><creatorcontrib>Gabuzda, D C</creatorcontrib><creatorcontrib>Jorstad, S G</creatorcontrib><creatorcontrib>Kudryavtseva, N A</creatorcontrib><creatorcontrib>Aller, M F</creatorcontrib><creatorcontrib>Aller, H D</creatorcontrib><creatorcontrib>Terasranta, H</creatorcontrib><title>The blazar 0059+581: Successful prognosis of activity</title><title>Astronomy reports</title><description>Our earlier joint analysis of light curves for the blazar 0059+581 at 4.8, 8, 14.5, 22, and 37 GHz with high-resolution VLBI images led us to suggest that the activity in this source develops in cycles, or periods, with a duration of about four years, with a 'typical scenario' for the development of the source's activity taking place over a cycle. Based on this analysis, we predicted in 2002 that a new superluminal component would be ejected from the core of this source in a structural position angle ~170DG no later than by the end of 2003. A 43-GHz VLBI image obtained on September 14, 2003, as part of a program to monitor the structure of reference sources used for a radio astronomical coordinate system, convincingly confirms the correctness of this prediction. This is the first time in the history of radio astronomy that a new superluminal component has been detected at a predicted time and in a predicted structural position angle.</description><subject>Astronomy</subject><subject>Astrophysics</subject><subject>Quasars</subject><subject>Radio astronomy</subject><issn>1063-7729</issn><issn>1562-6881</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2006</creationdate><recordtype>article</recordtype><recordid>eNqFkU1LA0EMhgdRsFZ_gLfFgx5kNTOZT29S_IKCh9bzMjs7q1u23TqzK9Rf75R6UtAkkEAe3iSEkFMKV5Qiv55RkKgUMyCTp9gjIyoky6XWdD_VqZ1v-4fkKMYFAKUa5YiI-ZvPytZ-2pABCHMpNL3JZoNzPsZ6aLN16F5XXWxi1tWZdX3z0fSbY3JQ2zb6k-88Ji_3d_PJYz59fnia3E5zh1L1OQfLdUkBjeC0rgQ3EpRVpXUWNTdGlNopb5VgTjBwVYWuRMkRK6s5CodjcrHTTVu8Dz72xbKJzretXfluiIUBhlwZrv8lFUfJDEuyY3L-J8mA8WSQwLMf4KIbwirdWyhhNGNabOfSHeRCF2PwdbEOzdKGTUGh2H6m-PUZ_AKtM3wx</recordid><startdate>20060601</startdate><enddate>20060601</enddate><creator>Pyatunina, T B</creator><creator>Gabuzda, D C</creator><creator>Jorstad, S G</creator><creator>Kudryavtseva, N A</creator><creator>Aller, M F</creator><creator>Aller, H D</creator><creator>Terasranta, H</creator><general>Springer Nature B.V</general><scope>AAYXX</scope><scope>CITATION</scope><scope>3V.</scope><scope>7TG</scope><scope>7XB</scope><scope>88I</scope><scope>8FD</scope><scope>8FE</scope><scope>8FG</scope><scope>8FK</scope><scope>ABUWG</scope><scope>AFKRA</scope><scope>ARAPS</scope><scope>AZQEC</scope><scope>BENPR</scope><scope>BGLVJ</scope><scope>CCPQU</scope><scope>DWQXO</scope><scope>GNUQQ</scope><scope>H8D</scope><scope>HCIFZ</scope><scope>KL.</scope><scope>L7M</scope><scope>M2P</scope><scope>P5Z</scope><scope>P62</scope><scope>PQEST</scope><scope>PQQKQ</scope><scope>PQUKI</scope><scope>Q9U</scope></search><sort><creationdate>20060601</creationdate><title>The blazar 0059+581: Successful prognosis of activity</title><author>Pyatunina, T B ; Gabuzda, D C ; Jorstad, S G ; Kudryavtseva, N A ; Aller, M F ; Aller, H D ; Terasranta, H</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c367t-40a48b1039541fd549607a7baca384995b8c7ea752c520cdd3cb36433da8435c3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2006</creationdate><topic>Astronomy</topic><topic>Astrophysics</topic><topic>Quasars</topic><topic>Radio astronomy</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Pyatunina, T B</creatorcontrib><creatorcontrib>Gabuzda, D C</creatorcontrib><creatorcontrib>Jorstad, S G</creatorcontrib><creatorcontrib>Kudryavtseva, N A</creatorcontrib><creatorcontrib>Aller, M F</creatorcontrib><creatorcontrib>Aller, H D</creatorcontrib><creatorcontrib>Terasranta, H</creatorcontrib><collection>CrossRef</collection><collection>ProQuest Central (Corporate)</collection><collection>Meteorological &amp; Geoastrophysical Abstracts</collection><collection>ProQuest Central (purchase pre-March 2016)</collection><collection>Science Database (Alumni Edition)</collection><collection>Technology Research Database</collection><collection>ProQuest SciTech Collection</collection><collection>ProQuest Technology Collection</collection><collection>ProQuest Central (Alumni) (purchase pre-March 2016)</collection><collection>ProQuest Central (Alumni)</collection><collection>ProQuest Central</collection><collection>Advanced Technologies &amp; Aerospace Collection</collection><collection>ProQuest Central Essentials</collection><collection>AUTh Library subscriptions: ProQuest Central</collection><collection>Technology Collection</collection><collection>ProQuest One Community College</collection><collection>ProQuest Central</collection><collection>ProQuest Central Student</collection><collection>Aerospace Database</collection><collection>SciTech Premium Collection</collection><collection>Meteorological &amp; Geoastrophysical Abstracts - Academic</collection><collection>Advanced Technologies Database with Aerospace</collection><collection>ProQuest Science Database</collection><collection>Advanced Technologies &amp; Aerospace Database</collection><collection>ProQuest Advanced Technologies &amp; Aerospace Collection</collection><collection>ProQuest One Academic Eastern Edition (DO NOT USE)</collection><collection>ProQuest One Academic</collection><collection>ProQuest One Academic UKI Edition</collection><collection>ProQuest Central Basic</collection><jtitle>Astronomy reports</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Pyatunina, T B</au><au>Gabuzda, D C</au><au>Jorstad, S G</au><au>Kudryavtseva, N A</au><au>Aller, M F</au><au>Aller, H D</au><au>Terasranta, H</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>The blazar 0059+581: Successful prognosis of activity</atitle><jtitle>Astronomy reports</jtitle><date>2006-06-01</date><risdate>2006</risdate><volume>50</volume><issue>6</issue><spage>468</spage><epage>482</epage><pages>468-482</pages><issn>1063-7729</issn><eissn>1562-6881</eissn><abstract>Our earlier joint analysis of light curves for the blazar 0059+581 at 4.8, 8, 14.5, 22, and 37 GHz with high-resolution VLBI images led us to suggest that the activity in this source develops in cycles, or periods, with a duration of about four years, with a 'typical scenario' for the development of the source's activity taking place over a cycle. Based on this analysis, we predicted in 2002 that a new superluminal component would be ejected from the core of this source in a structural position angle ~170DG no later than by the end of 2003. A 43-GHz VLBI image obtained on September 14, 2003, as part of a program to monitor the structure of reference sources used for a radio astronomical coordinate system, convincingly confirms the correctness of this prediction. This is the first time in the history of radio astronomy that a new superluminal component has been detected at a predicted time and in a predicted structural position angle.</abstract><cop>Heidelberg</cop><pub>Springer Nature B.V</pub><doi>10.1134/S1063772906060060</doi><tpages>15</tpages></addata></record>
fulltext fulltext
identifier ISSN: 1063-7729
ispartof Astronomy reports, 2006-06, Vol.50 (6), p.468-482
issn 1063-7729
1562-6881
language eng
recordid cdi_proquest_miscellaneous_902347948
source Springer Link
subjects Astronomy
Astrophysics
Quasars
Radio astronomy
title The blazar 0059+581: Successful prognosis of activity
url http://sfxeu10.hosted.exlibrisgroup.com/loughborough?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-01-05T01%3A15%3A24IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest_cross&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=The%20blazar%200059+581:%20Successful%20prognosis%20of%20activity&rft.jtitle=Astronomy%20reports&rft.au=Pyatunina,%20T%20B&rft.date=2006-06-01&rft.volume=50&rft.issue=6&rft.spage=468&rft.epage=482&rft.pages=468-482&rft.issn=1063-7729&rft.eissn=1562-6881&rft_id=info:doi/10.1134/S1063772906060060&rft_dat=%3Cproquest_cross%3E743629284%3C/proquest_cross%3E%3Cgrp_id%3Ecdi_FETCH-LOGICAL-c367t-40a48b1039541fd549607a7baca384995b8c7ea752c520cdd3cb36433da8435c3%3C/grp_id%3E%3Coa%3E%3C/oa%3E%3Curl%3E%3C/url%3E&rft_id=info:oai/&rft_pqid=759822858&rft_id=info:pmid/&rfr_iscdi=true