Empirical sigma - d relations and main galactic radio loops

This paper represents a review of the empirical Galactic and extragalactic sigma - D relations (relations between the surface brightness sigma and the diameter D) for supernova remnants (SNRs), with checking the connection of the main Galactic radio loops (Loop I, II, III and IV) with these relation...

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Main Author: Urošević Dejan V.
Format: Article
Language:English
Published: Astronomical Observatory, Department of Astronomy, Belgrade 2002-01-01
Series:Serbian Astronomical Journal
Online Access:http://www.doiserbia.nb.rs/img/doi/1450-698X/2002/1450-698X0265027U.pdf
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author Urošević Dejan V.
author_facet Urošević Dejan V.
author_sort Urošević Dejan V.
collection DOAJ
description This paper represents a review of the empirical Galactic and extragalactic sigma - D relations (relations between the surface brightness sigma and the diameter D) for supernova remnants (SNRs), with checking the connection of the main Galactic radio loops (Loop I, II, III and IV) with these relations. We present results which suggest, in another way, that the radio loops may have an SNR origin. The updated relations have been measured to have slopes beta = 2 in log-log space. The best sigma - D relations for M31 and M33 galaxies were derived and these relations are shown to be flatter (beta < 2) than those for Galactic SNRs alone. This result confirms that selection effects play an important role in data-sets made up of Galactic SNRs. A sigma - D relation with 157 reliable calibrators (both Galactic and extragalactic) is derived. This relation also has a slope beta = 2.07 ± 13.
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spelling doaj.art-90155b1063454703bf1399652d4ff03f2022-12-22T03:21:27ZengAstronomical Observatory, Department of Astronomy, BelgradeSerbian Astronomical Journal1450-698X1820-92892002-01-012002165274310.2298/SAJ0265027U1450-698X0265027UEmpirical sigma - d relations and main galactic radio loopsUrošević Dejan V.0Katedra za astronomiju, Matematički fakultet, Univerzitet u BeograduThis paper represents a review of the empirical Galactic and extragalactic sigma - D relations (relations between the surface brightness sigma and the diameter D) for supernova remnants (SNRs), with checking the connection of the main Galactic radio loops (Loop I, II, III and IV) with these relations. We present results which suggest, in another way, that the radio loops may have an SNR origin. The updated relations have been measured to have slopes beta = 2 in log-log space. The best sigma - D relations for M31 and M33 galaxies were derived and these relations are shown to be flatter (beta < 2) than those for Galactic SNRs alone. This result confirms that selection effects play an important role in data-sets made up of Galactic SNRs. A sigma - D relation with 157 reliable calibrators (both Galactic and extragalactic) is derived. This relation also has a slope beta = 2.07 ± 13.http://www.doiserbia.nb.rs/img/doi/1450-698X/2002/1450-698X0265027U.pdf
spellingShingle Urošević Dejan V.
Empirical sigma - d relations and main galactic radio loops
Serbian Astronomical Journal
title Empirical sigma - d relations and main galactic radio loops
title_full Empirical sigma - d relations and main galactic radio loops
title_fullStr Empirical sigma - d relations and main galactic radio loops
title_full_unstemmed Empirical sigma - d relations and main galactic radio loops
title_short Empirical sigma - d relations and main galactic radio loops
title_sort empirical sigma d relations and main galactic radio loops
url http://www.doiserbia.nb.rs/img/doi/1450-698X/2002/1450-698X0265027U.pdf
work_keys_str_mv AT urosevicdejanv empiricalsigmadrelationsandmaingalacticradioloops