A search for radio supernovae and supernova remnants in the region of NGC 1569's super star clusters

A. Greve; A. Tarchi; S. Hüttemeister; R. de Grijs; J. M. Van Der Hulst; S. T. Garrington; N. Neininger

doi:10.1051/0004-6361:20011467

A search for radio supernovae and supernova remnants in the region of NGC 1569's super star clusters

A. Greve^*, A. Tarchi, S. Hüttemeister, R. de Grijs, J. M. Van Der Hulst, S. T. Garrington, N. Neininger

^*Corresponding author for this work

Research output: Contribution to journal › Article › peer-review

28 Citations (Scopus)

Abstract

We have used MERLIN, at 1.4 and 5 GHz, to search for radio supernovae (RSNe) and supernova remnants (SNRs) in the unobscured irregular dwarf galaxy NGC 1569, and in particular in the region of its super star clusters (SSCs) A and B. Throughout NGC 1569 we find some 5 RSNe and SNRs but the SSCs and their immediate surroundings are largely devoid of non-thermal radio sources. Even though many massive stars in the SSCs are expected to have exploded already, when compared with M 82 and its many SSCs the absence of RSNe and SNRs in and near A and B may seem plausible on statistical arguments. The absence of RSNe and SNRs in and near A and B may, however, also be due to a violent and turbulent outflow of stellar winds and supernova ejected material, which does not provide a quiescent environment for the development of SNRs within and near the SSCs.

Original language	English
Pages (from-to)	825-833
Number of pages	9
Journal	Astronomy and Astrophysics
Volume	381
Issue number	3
DOIs	https://doi.org/10.1051/0004-6361:20011467
Publication status	Published - Jan 2002
Externally published	Yes

Keywords

galaxies: individual: NGC 1569
galaxies: ISM

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10.1051/0004-6361:20011467

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title = "A search for radio supernovae and supernova remnants in the region of NGC 1569's super star clusters",

abstract = "We have used MERLIN, at 1.4 and 5 GHz, to search for radio supernovae (RSNe) and supernova remnants (SNRs) in the unobscured irregular dwarf galaxy NGC 1569, and in particular in the region of its super star clusters (SSCs) A and B. Throughout NGC 1569 we find some 5 RSNe and SNRs but the SSCs and their immediate surroundings are largely devoid of non-thermal radio sources. Even though many massive stars in the SSCs are expected to have exploded already, when compared with M 82 and its many SSCs the absence of RSNe and SNRs in and near A and B may seem plausible on statistical arguments. The absence of RSNe and SNRs in and near A and B may, however, also be due to a violent and turbulent outflow of stellar winds and supernova ejected material, which does not provide a quiescent environment for the development of SNRs within and near the SSCs.",

keywords = "galaxies: individual: NGC 1569, galaxies: ISM",

author = "A. Greve and A. Tarchi and S. H{\"u}ttemeister and {de Grijs}, R. and {Van Der Hulst}, {J. M.} and Garrington, {S. T.} and N. Neininger",

year = "2002",

month = jan,

doi = "10.1051/0004-6361:20011467",

language = "English",

volume = "381",

pages = "825--833",

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T1 - A search for radio supernovae and supernova remnants in the region of NGC 1569's super star clusters

AU - Greve, A.

AU - Tarchi, A.

AU - Hüttemeister, S.

AU - de Grijs, R.

AU - Van Der Hulst, J. M.

AU - Garrington, S. T.

AU - Neininger, N.

PY - 2002/1

Y1 - 2002/1

N2 - We have used MERLIN, at 1.4 and 5 GHz, to search for radio supernovae (RSNe) and supernova remnants (SNRs) in the unobscured irregular dwarf galaxy NGC 1569, and in particular in the region of its super star clusters (SSCs) A and B. Throughout NGC 1569 we find some 5 RSNe and SNRs but the SSCs and their immediate surroundings are largely devoid of non-thermal radio sources. Even though many massive stars in the SSCs are expected to have exploded already, when compared with M 82 and its many SSCs the absence of RSNe and SNRs in and near A and B may seem plausible on statistical arguments. The absence of RSNe and SNRs in and near A and B may, however, also be due to a violent and turbulent outflow of stellar winds and supernova ejected material, which does not provide a quiescent environment for the development of SNRs within and near the SSCs.

AB - We have used MERLIN, at 1.4 and 5 GHz, to search for radio supernovae (RSNe) and supernova remnants (SNRs) in the unobscured irregular dwarf galaxy NGC 1569, and in particular in the region of its super star clusters (SSCs) A and B. Throughout NGC 1569 we find some 5 RSNe and SNRs but the SSCs and their immediate surroundings are largely devoid of non-thermal radio sources. Even though many massive stars in the SSCs are expected to have exploded already, when compared with M 82 and its many SSCs the absence of RSNe and SNRs in and near A and B may seem plausible on statistical arguments. The absence of RSNe and SNRs in and near A and B may, however, also be due to a violent and turbulent outflow of stellar winds and supernova ejected material, which does not provide a quiescent environment for the development of SNRs within and near the SSCs.

KW - galaxies: individual: NGC 1569

KW - galaxies: ISM

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U2 - 10.1051/0004-6361:20011467

DO - 10.1051/0004-6361:20011467

M3 - Article

AN - SCOPUS:0036188629

SN - 0004-6361

VL - 381

SP - 825

EP - 833

JO - Astronomy and Astrophysics

JF - Astronomy and Astrophysics

IS - 3

ER -

A search for radio supernovae and supernova remnants in the region of NGC 1569's super star clusters

Abstract

Keywords

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