Monitoring of the Prompt Radio Emission from the Unusual Supernova SN 2004dj in NGC 2403

Supernova SN 2004dj in the nearby spiral galaxy NGC 2403 was detected optically in 2004 July. Peaking at a magnitude of 11.2, this is the brightest supernova detected for several years. Here we present Multi-Element Radio Linked Interferometer Network (MERLIN) observations of this source, made over...

Full description

Bibliographic Details
Main Authors: Beswick, R, Muxlow, T, Argo, Megan, Pedlar, A, Marcaide, J, Wills, K
Format: Journal Article
Published: The American Astronomical Society 2005
Subjects:
Online Access:http://hdl.handle.net/20.500.11937/40435
_version_ 1848755870791368704
author Beswick, R
Muxlow, T
Argo, Megan
Pedlar, A
Marcaide, J
Wills, K
author_facet Beswick, R
Muxlow, T
Argo, Megan
Pedlar, A
Marcaide, J
Wills, K
author_sort Beswick, R
building Curtin Institutional Repository
collection Online Access
description Supernova SN 2004dj in the nearby spiral galaxy NGC 2403 was detected optically in 2004 July. Peaking at a magnitude of 11.2, this is the brightest supernova detected for several years. Here we present Multi-Element Radio Linked Interferometer Network (MERLIN) observations of this source, made over a 4 month period, that give a position of R.A. = 07h37m17.s044, decl. = +65 35' 57".84 (J2000.0). We also present a well-sampled 5 GHz light curve covering the period from 2004 August 5 to December 2. With the exception of the unusual and very close SN 1987A, these observations represent the first detailed radio light curve for the prompt emission from a Type II-P supernova.
first_indexed 2025-11-14T09:03:11Z
format Journal Article
id curtin-20.500.11937-40435
institution Curtin University Malaysia
institution_category Local University
last_indexed 2025-11-14T09:03:11Z
publishDate 2005
publisher The American Astronomical Society
recordtype eprints
repository_type Digital Repository
spelling curtin-20.500.11937-404352023-02-22T06:24:24Z Monitoring of the Prompt Radio Emission from the Unusual Supernova SN 2004dj in NGC 2403 Beswick, R Muxlow, T Argo, Megan Pedlar, A Marcaide, J Wills, K starburst galaxies radio continuum supernovae stars SN 2004dj) individual (SN 2004dj Supernova SN 2004dj in the nearby spiral galaxy NGC 2403 was detected optically in 2004 July. Peaking at a magnitude of 11.2, this is the brightest supernova detected for several years. Here we present Multi-Element Radio Linked Interferometer Network (MERLIN) observations of this source, made over a 4 month period, that give a position of R.A. = 07h37m17.s044, decl. = +65 35' 57".84 (J2000.0). We also present a well-sampled 5 GHz light curve covering the period from 2004 August 5 to December 2. With the exception of the unusual and very close SN 1987A, these observations represent the first detailed radio light curve for the prompt emission from a Type II-P supernova. 2005 Journal Article http://hdl.handle.net/20.500.11937/40435 10.1086/430049 The American Astronomical Society unknown
spellingShingle starburst
galaxies
radio continuum
supernovae
stars
SN 2004dj)
individual (SN 2004dj
Beswick, R
Muxlow, T
Argo, Megan
Pedlar, A
Marcaide, J
Wills, K
Monitoring of the Prompt Radio Emission from the Unusual Supernova SN 2004dj in NGC 2403
title Monitoring of the Prompt Radio Emission from the Unusual Supernova SN 2004dj in NGC 2403
title_full Monitoring of the Prompt Radio Emission from the Unusual Supernova SN 2004dj in NGC 2403
title_fullStr Monitoring of the Prompt Radio Emission from the Unusual Supernova SN 2004dj in NGC 2403
title_full_unstemmed Monitoring of the Prompt Radio Emission from the Unusual Supernova SN 2004dj in NGC 2403
title_short Monitoring of the Prompt Radio Emission from the Unusual Supernova SN 2004dj in NGC 2403
title_sort monitoring of the prompt radio emission from the unusual supernova sn 2004dj in ngc 2403
topic starburst
galaxies
radio continuum
supernovae
stars
SN 2004dj)
individual (SN 2004dj
url http://hdl.handle.net/20.500.11937/40435