MODIFIED EQUIPARTITION CALCULATION FOR SUPERNOVA REMNANTS. CASES α = 0.5 AND α = 1

The equipartition or minimum energy calculation is a well-known procedure for estimating the magnetic field strength and the total energy in the magnetic field and cosmic ray particles by using only the radio synchrotron emission. In one of our previous papers, we have offered a modified equipartiti...

Ausführliche Beschreibung

Gespeichert in:

Bibliographische Detailangaben
Veröffentlicht in:	The Astrophysical journal 2013-11, Vol.777 (1), p.1-3
Hauptverfasser:	ARBUTINA, B, Urosevic, D, Vucetic, M M, Pavlovic, M Z, VUKOTIC, B
Format:	Artikel
Sprache:	eng
Schlagworte:	ASTRONOMY ASTROPHYSICS ASTROPHYSICS, COSMOLOGY AND ASTRONOMY COSMIC RADIATION Emission Energy use MAGNETIC FIELDS Mathematical analysis Spectra Strength SUPERNOVA REMNANTS Synchrotrons
Online-Zugang:	Volltext
Tags:	Tag hinzufügen Keine Tags, Fügen Sie den ersten Tag hinzu!

container_end_page	3
container_issue	1
container_start_page	1
container_title	The Astrophysical journal
container_volume	777
creator	ARBUTINA, B Urosevic, D Vucetic, M M Pavlovic, M Z VUKOTIC, B
description	The equipartition or minimum energy calculation is a well-known procedure for estimating the magnetic field strength and the total energy in the magnetic field and cosmic ray particles by using only the radio synchrotron emission. In one of our previous papers, we have offered a modified equipartition calculation for supernova remnants (SNRs) with spectral indices 0.5 < alpha < 1. Here we extend the analysis to SNRs with alpha = 0.5 and alpha = 1.
doi_str_mv	10.1088/0004-637X/777/1/31
format	Article
fullrecord	<record><control><sourceid>proquest_osti_</sourceid><recordid>TN_cdi_osti_scitechconnect_22270691</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>1718964827</sourcerecordid><originalsourceid>FETCH-LOGICAL-c385t-df09345bad79636791cf3c6aa2e0b3a2bcb588564701ee7cc8e11654fb5d287b3</originalsourceid><addsrcrecordid>eNqN0ctOg0AUBuCJ0cRafQFXJG7cUObCXFi4IC1VkhYqF-NuAtMhYtqiDF34WL6IzySIce3qnD_5chb_AeAawRmCQjgQQtdmhD87nHMHOQSdgAmiRNguofwUTP7AObgw5nWI2PMmIFvHi3AZBgsreMzDjZ9kYRbGkTX3V_N85f_syzix0nwTJFH85FtJsI78KEtnvUmD1Pr6tO4sOKOWHy3GgC7BWVXsjL76nVOQL4Ns_mCv4vuwv2wrImhnbyvoEZeWxZZ7jDDuIVURxYoCa1iSApeqpEJQ5nKItOZKCY0Qo25V0i0WvCRTcDPebUxXS6PqTqsX1RwOWnUSY8wh81Cvbkf11jbvR206ua-N0rtdcdDN0UjEkfCYKzD_B4UUCi6E21M8UtU2xrS6km9tvS_aD4mgHH4ih47lULnsfyKRJIh8A4tYdvA</addsrcrecordid><sourcetype>Open Access Repository</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>1705087884</pqid></control><display><type>article</type><title>MODIFIED EQUIPARTITION CALCULATION FOR SUPERNOVA REMNANTS. CASES α = 0.5 AND α = 1</title><source>IOP Publishing Free Content</source><source>Elektronische Zeitschriftenbibliothek - Frei zugängliche E-Journals</source><source>Alma/SFX Local Collection</source><creator>ARBUTINA, B ; Urosevic, D ; Vucetic, M M ; Pavlovic, M Z ; VUKOTIC, B</creator><creatorcontrib>ARBUTINA, B ; Urosevic, D ; Vucetic, M M ; Pavlovic, M Z ; VUKOTIC, B</creatorcontrib><description>The equipartition or minimum energy calculation is a well-known procedure for estimating the magnetic field strength and the total energy in the magnetic field and cosmic ray particles by using only the radio synchrotron emission. In one of our previous papers, we have offered a modified equipartition calculation for supernova remnants (SNRs) with spectral indices 0.5 < alpha < 1. Here we extend the analysis to SNRs with alpha = 0.5 and alpha = 1.</description><identifier>ISSN: 0004-637X</identifier><identifier>EISSN: 1538-4357</identifier><identifier>DOI: 10.1088/0004-637X/777/1/31</identifier><language>eng</language><publisher>United States</publisher><subject>ASTRONOMY ; ASTROPHYSICS ; ASTROPHYSICS, COSMOLOGY AND ASTRONOMY ; COSMIC RADIATION ; Emission ; Energy use ; MAGNETIC FIELDS ; Mathematical analysis ; Spectra ; Strength ; SUPERNOVA REMNANTS ; Synchrotrons</subject><ispartof>The Astrophysical journal, 2013-11, Vol.777 (1), p.1-3</ispartof><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c385t-df09345bad79636791cf3c6aa2e0b3a2bcb588564701ee7cc8e11654fb5d287b3</citedby><cites>FETCH-LOGICAL-c385t-df09345bad79636791cf3c6aa2e0b3a2bcb588564701ee7cc8e11654fb5d287b3</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>230,314,780,784,885,27923,27924</link.rule.ids><backlink>$$Uhttps://www.osti.gov/biblio/22270691$$D View this record in Osti.gov$$Hfree_for_read</backlink></links><search><creatorcontrib>ARBUTINA, B</creatorcontrib><creatorcontrib>Urosevic, D</creatorcontrib><creatorcontrib>Vucetic, M M</creatorcontrib><creatorcontrib>Pavlovic, M Z</creatorcontrib><creatorcontrib>VUKOTIC, B</creatorcontrib><title>MODIFIED EQUIPARTITION CALCULATION FOR SUPERNOVA REMNANTS. CASES α = 0.5 AND α = 1</title><title>The Astrophysical journal</title><description>The equipartition or minimum energy calculation is a well-known procedure for estimating the magnetic field strength and the total energy in the magnetic field and cosmic ray particles by using only the radio synchrotron emission. In one of our previous papers, we have offered a modified equipartition calculation for supernova remnants (SNRs) with spectral indices 0.5 < alpha < 1. Here we extend the analysis to SNRs with alpha = 0.5 and alpha = 1.</description><subject>ASTRONOMY</subject><subject>ASTROPHYSICS</subject><subject>ASTROPHYSICS, COSMOLOGY AND ASTRONOMY</subject><subject>COSMIC RADIATION</subject><subject>Emission</subject><subject>Energy use</subject><subject>MAGNETIC FIELDS</subject><subject>Mathematical analysis</subject><subject>Spectra</subject><subject>Strength</subject><subject>SUPERNOVA REMNANTS</subject><subject>Synchrotrons</subject><issn>0004-637X</issn><issn>1538-4357</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2013</creationdate><recordtype>article</recordtype><recordid>eNqN0ctOg0AUBuCJ0cRafQFXJG7cUObCXFi4IC1VkhYqF-NuAtMhYtqiDF34WL6IzySIce3qnD_5chb_AeAawRmCQjgQQtdmhD87nHMHOQSdgAmiRNguofwUTP7AObgw5nWI2PMmIFvHi3AZBgsreMzDjZ9kYRbGkTX3V_N85f_syzix0nwTJFH85FtJsI78KEtnvUmD1Pr6tO4sOKOWHy3GgC7BWVXsjL76nVOQL4Ns_mCv4vuwv2wrImhnbyvoEZeWxZZ7jDDuIVURxYoCa1iSApeqpEJQ5nKItOZKCY0Qo25V0i0WvCRTcDPebUxXS6PqTqsX1RwOWnUSY8wh81Cvbkf11jbvR206ua-N0rtdcdDN0UjEkfCYKzD_B4UUCi6E21M8UtU2xrS6km9tvS_aD4mgHH4ih47lULnsfyKRJIh8A4tYdvA</recordid><startdate>20131101</startdate><enddate>20131101</enddate><creator>ARBUTINA, B</creator><creator>Urosevic, D</creator><creator>Vucetic, M M</creator><creator>Pavlovic, M Z</creator><creator>VUKOTIC, B</creator><scope>AAYXX</scope><scope>CITATION</scope><scope>7TG</scope><scope>KL.</scope><scope>8FD</scope><scope>H8D</scope><scope>L7M</scope><scope>OTOTI</scope></search><sort><creationdate>20131101</creationdate><title>MODIFIED EQUIPARTITION CALCULATION FOR SUPERNOVA REMNANTS. CASES α = 0.5 AND α = 1</title><author>ARBUTINA, B ; Urosevic, D ; Vucetic, M M ; Pavlovic, M Z ; VUKOTIC, B</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c385t-df09345bad79636791cf3c6aa2e0b3a2bcb588564701ee7cc8e11654fb5d287b3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2013</creationdate><topic>ASTRONOMY</topic><topic>ASTROPHYSICS</topic><topic>ASTROPHYSICS, COSMOLOGY AND ASTRONOMY</topic><topic>COSMIC RADIATION</topic><topic>Emission</topic><topic>Energy use</topic><topic>MAGNETIC FIELDS</topic><topic>Mathematical analysis</topic><topic>Spectra</topic><topic>Strength</topic><topic>SUPERNOVA REMNANTS</topic><topic>Synchrotrons</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>ARBUTINA, B</creatorcontrib><creatorcontrib>Urosevic, D</creatorcontrib><creatorcontrib>Vucetic, M M</creatorcontrib><creatorcontrib>Pavlovic, M Z</creatorcontrib><creatorcontrib>VUKOTIC, B</creatorcontrib><collection>CrossRef</collection><collection>Meteorological & Geoastrophysical Abstracts</collection><collection>Meteorological & Geoastrophysical Abstracts - Academic</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Advanced Technologies Database with Aerospace</collection><collection>OSTI.GOV</collection><jtitle>The Astrophysical journal</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>ARBUTINA, B</au><au>Urosevic, D</au><au>Vucetic, M M</au><au>Pavlovic, M Z</au><au>VUKOTIC, B</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>MODIFIED EQUIPARTITION CALCULATION FOR SUPERNOVA REMNANTS. CASES α = 0.5 AND α = 1</atitle><jtitle>The Astrophysical journal</jtitle><date>2013-11-01</date><risdate>2013</risdate><volume>777</volume><issue>1</issue><spage>1</spage><epage>3</epage><pages>1-3</pages><issn>0004-637X</issn><eissn>1538-4357</eissn><abstract>The equipartition or minimum energy calculation is a well-known procedure for estimating the magnetic field strength and the total energy in the magnetic field and cosmic ray particles by using only the radio synchrotron emission. In one of our previous papers, we have offered a modified equipartition calculation for supernova remnants (SNRs) with spectral indices 0.5 < alpha < 1. Here we extend the analysis to SNRs with alpha = 0.5 and alpha = 1.</abstract><cop>United States</cop><doi>10.1088/0004-637X/777/1/31</doi><tpages>3</tpages><oa>free_for_read</oa></addata></record>
fulltext	fulltext
identifier	ISSN: 0004-637X
ispartof	The Astrophysical journal, 2013-11, Vol.777 (1), p.1-3
issn	0004-637X 1538-4357
language	eng
recordid	cdi_osti_scitechconnect_22270691
source	IOP Publishing Free Content; Elektronische Zeitschriftenbibliothek - Frei zugängliche E-Journals; Alma/SFX Local Collection
subjects	ASTRONOMY ASTROPHYSICS ASTROPHYSICS, COSMOLOGY AND ASTRONOMY COSMIC RADIATION Emission Energy use MAGNETIC FIELDS Mathematical analysis Spectra Strength SUPERNOVA REMNANTS Synchrotrons
title	MODIFIED EQUIPARTITION CALCULATION FOR SUPERNOVA REMNANTS. CASES α = 0.5 AND α = 1
url	https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-01-08T16%3A59%3A16IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest_osti_&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=MODIFIED%20EQUIPARTITION%20CALCULATION%20FOR%20SUPERNOVA%20REMNANTS.%20CASES%20%CE%B1%20=%200.5%20AND%20%CE%B1%20=%201&rft.jtitle=The%20Astrophysical%20journal&rft.au=ARBUTINA,%20B&rft.date=2013-11-01&rft.volume=777&rft.issue=1&rft.spage=1&rft.epage=3&rft.pages=1-3&rft.issn=0004-637X&rft.eissn=1538-4357&rft_id=info:doi/10.1088/0004-637X/777/1/31&rft_dat=%3Cproquest_osti_%3E1718964827%3C/proquest_osti_%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_pqid=1705087884&rft_id=info:pmid/&rfr_iscdi=true