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A MeerKAT morphological and spectral index study of M87

Dissertation (MSc (Physics))--University of Pretoria, 2022.

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Other Authors: Dean, Roger
Format: Thesis
Language:English
Published: University of Pretoria 2022
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access_status_str Open Access
author2 Dean, Roger
author_browse Dean, Roger
author_facet Dean, Roger
collection Thesis
dc_rights_str_mv © 2022 University of Pretoria. All rights reserved. The copyright in this work vests in the University of Pretoria. No part of this work may be reproduced or transmitted in any form or by any means, without the prior written permission of the University of Pretoria.
description Dissertation (MSc (Physics))--University of Pretoria, 2022.
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institution University of Pretoria (South Africa)
language English
last_indexed 2026-06-10T12:37:30.755Z
license_str Other — see source repository
provenance_str_mv Harvested via OAI-PMH from UPSpace — University of Pretoria Institutional Repository
publishDate 2022
publishDateRange 2022
publishDateSort 2022
publisher University of Pretoria
publisherStr University of Pretoria
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spelling oai:repository.up.ac.za:2263/86434 A MeerKAT morphological and spectral index study of M87 Dean, Roger u13371062@tuks.co.za Thorat, Kshitij Mtshweni, Leon MeerKAT Astronomy Radio survey Messier 87 Spectral indices UCTD Dissertation (MSc (Physics))--University of Pretoria, 2022. Messier 87 (M87) is a spectacular radio galaxy located in our cosmic backyard. Its proximity has allowed astronomers to study it in detail across the electromagnetic spectrum. M87 shows a complex structure in the radio continuum made up of a bright core, jets and a diffuse halo. High fidelity imaging of this bright (> 300$\, $Jy), complex source is necessary to understanding its evolution. MeerKAT’s sensitivity and spatial resolution make it an ideal instrument to study M87's extended, diffuse radio structure. We present the MeerKAT 1.28$\, $GHz total-intensity map, in-band spectral index image, and an analysis of its complex morphological structure. A comparison of the MeerKAT map with the VLA map is conducted, comparing all key features, by means of a two point spectral index map at the respective frequencies, 1.28$\, $GHz and 327$\, $MHz. Our results 1) verify the structures seen in the VLA 327$\, $MHz image, made using maximum entropy techniques 2) show the first spectral index of the filamentary structures 3) demonstrate the ability of MeerKAT to map complex, diffuse structures at higher frequencies than before, extending the frequency range to enable for more detailed, spatially resolved spectral analysis. In conclusion, we find results that are consistent with what has been observed about M87, that it is an active galaxy with a steady spectral variation across a large radio frequency range. SARAO NRF IDIA Physics MSc (Physics) Unrestricted 2022-07-25T10:46:20Z 2022-07-25T10:46:20Z 2022-09-06 2022-03-29 Dissertation * S2022 https://repository.up.ac.za/handle/2263/86434 https://doi.org/10.25403/UPresearchdata.20358261 en © 2022 University of Pretoria. All rights reserved. The copyright in this work vests in the University of Pretoria. No part of this work may be reproduced or transmitted in any form or by any means, without the prior written permission of the University of Pretoria. application/pdf University of Pretoria
spellingShingle MeerKAT
Astronomy
Radio survey
Messier 87
Spectral indices
UCTD
A MeerKAT morphological and spectral index study of M87
title A MeerKAT morphological and spectral index study of M87
title_full A MeerKAT morphological and spectral index study of M87
title_fullStr A MeerKAT morphological and spectral index study of M87
title_full_unstemmed A MeerKAT morphological and spectral index study of M87
title_short A MeerKAT morphological and spectral index study of M87
title_sort meerkat morphological and spectral index study of m87
topic MeerKAT
Astronomy
Radio survey
Messier 87
Spectral indices
UCTD
url https://repository.up.ac.za/handle/2263/86434
https://doi.org/10.25403/UPresearchdata.20358261