On the integrated continuum radio spectrum of supernova remnant W44 (G34.7-0.4): New insights from Planck

In this paper, the integrated continuum radio spectrum of supernova remnant (SNR) W44 was analyzed up to 70 GHz, testing the different emission models that can be responsible for its particular shape. The observations by the Planck space telescope made it possible to analyze the high freque...

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Main Author: Onić D.
Format: Article
Language:English
Published: Astronomical Observatory, Department of Astronomy, Belgrade 2015-01-01
Series:Serbian Astronomical Journal
Subjects:
Online Access:http://www.doiserbia.nb.rs/img/doi/1450-698X/2015/1450-698X1500004O.pdf
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author Onić D.
author_facet Onić D.
author_sort Onić D.
collection DOAJ
description In this paper, the integrated continuum radio spectrum of supernova remnant (SNR) W44 was analyzed up to 70 GHz, testing the different emission models that can be responsible for its particular shape. The observations by the Planck space telescope made it possible to analyze the high frequency part of radio emission from SNRs. Although the quality of radio continuum spectrum (a high scatter of data points at same frequencies) prevents us to make definite conclusions, the possibility of spinning dust emission detection towards this remnant is emphasized. In addition, a concave-down feature, due to synchrotron losses, can not be definitely dismissed by the present knowledge of the integrated radio continuum spectrum of this SNR. [Projekat Ministarstva nauke Republike Srbije, br. 176005: Emission Nebulae: Structure and Evolution]
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spelling doaj.art-fccdedae686943838c0c6569680dbd092022-12-22T01:56:27ZengAstronomical Observatory, Department of Astronomy, BelgradeSerbian Astronomical Journal1450-698X1820-92892015-01-012015191293710.2298/SAJ150715004O1450-698X1500004OOn the integrated continuum radio spectrum of supernova remnant W44 (G34.7-0.4): New insights from PlanckOnić D.0Faculty of Mathematics, Department of Astronomy, BelgradeIn this paper, the integrated continuum radio spectrum of supernova remnant (SNR) W44 was analyzed up to 70 GHz, testing the different emission models that can be responsible for its particular shape. The observations by the Planck space telescope made it possible to analyze the high frequency part of radio emission from SNRs. Although the quality of radio continuum spectrum (a high scatter of data points at same frequencies) prevents us to make definite conclusions, the possibility of spinning dust emission detection towards this remnant is emphasized. In addition, a concave-down feature, due to synchrotron losses, can not be definitely dismissed by the present knowledge of the integrated radio continuum spectrum of this SNR. [Projekat Ministarstva nauke Republike Srbije, br. 176005: Emission Nebulae: Structure and Evolution]http://www.doiserbia.nb.rs/img/doi/1450-698X/2015/1450-698X1500004O.pdfISM: individual (W44)ISM: supernova remnantsradio continuum: ISM
spellingShingle Onić D.
On the integrated continuum radio spectrum of supernova remnant W44 (G34.7-0.4): New insights from Planck
Serbian Astronomical Journal
ISM: individual (W44)
ISM: supernova remnants
radio continuum: ISM
title On the integrated continuum radio spectrum of supernova remnant W44 (G34.7-0.4): New insights from Planck
title_full On the integrated continuum radio spectrum of supernova remnant W44 (G34.7-0.4): New insights from Planck
title_fullStr On the integrated continuum radio spectrum of supernova remnant W44 (G34.7-0.4): New insights from Planck
title_full_unstemmed On the integrated continuum radio spectrum of supernova remnant W44 (G34.7-0.4): New insights from Planck
title_short On the integrated continuum radio spectrum of supernova remnant W44 (G34.7-0.4): New insights from Planck
title_sort on the integrated continuum radio spectrum of supernova remnant w44 g34 7 0 4 new insights from planck
topic ISM: individual (W44)
ISM: supernova remnants
radio continuum: ISM
url http://www.doiserbia.nb.rs/img/doi/1450-698X/2015/1450-698X1500004O.pdf
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