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volume 534 issue 3 pages 2918-2937

Discovery of Perun (G329.9-0.5): A New, Young, Galactic SNR

Zachary J. Smeaton 1, 2
Miroslav D. Filipović 1
M. D. Filipović 2
Sanja Lazarević 2, 3, 4
R. Z. E. Alsaberi 1, 2
Adeel Ahmad 2
M. Araya 5
Brianna D Ball 6
C. Bordiu 7, 8
Carla S. Buemi 7
C. Buemi 8
Filomena Bufano 8
S. Dai 1, 2, 3
Frank Haberl 9
Andrew M Hopkins 10
Andrew Hopkins 11
Adriano Ingallinera 8
Thomas Jarrett 1, 12
T. H. Jarrett 2, 13
Bärbel S Koribalski 1, 14
B. Koribalski 2, 3
Roland Kothes 15
Renée C. Kraan-Korteweg 12
R. C. Kraan-Korteweg 13
Denis Leahy 16
D. A. Leahy 17
Peter Lundqvist 18
Chandreyee Maitra 9
Pierrick Martin 19
J L Payne 1, 2
Gavin Rowell 20
G. P. Rowell 21
Hidetoshi Sano 22, 23
M. Sasaki 24, 25
Roberto Soria 26, 27
Nadia Steyn 28, 29
Grazia Umana 7
G. Umana 8
Dejan Urošević 30
D. Urošević 31
Velibor Velović 2
T. Vernstrom 28, 29, 32, 33
Branislav Vukotić 34
B. Vukotić 4
J. L. West 15, 35
4
 
Astronomical Observatory , Volgina 7, 11060 Belgrade ,
34
 
Astronomical Observatory , Volgina 7, 11060 Belgrade,
Publication typeJournal Article
Publication date2024-09-30
scimago Q1
wos Q1
SJR1.702
CiteScore9.7
Impact factor4.8
ISSN00358711, 13652966, 13658711
Abstract
ABSTRACT

We present the discovery of possibly the youngest Galactic supernova remnant (SNR) with associated pulsar-wind nebula (PWN), which we name Perun (G329.9−0.5). Perun was serendipitously discovered in the Australian Square Kilometre Array Pathfinder–Evolutionary Map of the Universe survey at 943 MHz, and subsequent follow-up observations were conducted with the Australia Telescope Compact Array observatory at 5500 and 9000 MHz. We combine these with additional radio observations from the MeerKAT, Molonglo Observatory Synthesis Telescope, and Murchison Widefield Array telescopes, infrared (IR) observations from the SpitzerSpace Telescope, and X-ray observations from the Chandra X-ray observatory to perform a multifrequency analysis. The radio morphology shows a small angular size shell (D = 70 arcsec) with a luminous, central PWN. We measure a total spectral index of $\alpha = -0.49\pm 0.05$, which should be typical for a young, composite SNR. Crucial evidence for Perun’s SNR classification comes from the detection of linear fractional polarization at radio frequencies of $\sim$7 per cent–10 per cent with both radial and tangential orientations, similar to the young SNR G1.9+0.3. We use data from the Southern Galactic Plane Survey to perform an H i analysis and estimate a favoured distance range of 6–9 kpc, and thus a favoured age range of $\sim$70–500 yr. We find no high-energy emission in Fermi-Large Area Telescope data. We detect Perun’s outer shell in 24 $\mu$m indicating the possible presence of [O iv] and [Fe iii] emission, also typical for young SNRs. Overall, these observations and analysis confirm Perun as a young, Galactic SNR with a prominent PWN.

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Smeaton Z. J. et al. Discovery of Perun (G329.9-0.5): A New, Young, Galactic SNR // Monthly Notices of the Royal Astronomical Society. 2024. Vol. 534. No. 3. pp. 2918-2937.
GOST all authors (up to 50) Copy
Smeaton Z. J. et al. Discovery of Perun (G329.9-0.5): A New, Young, Galactic SNR // Monthly Notices of the Royal Astronomical Society. 2024. Vol. 534. No. 3. pp. 2918-2937.
RIS |
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RIS Copy
TY - JOUR
DO - 10.1093/mnras/stae2237
UR - https://academic.oup.com/mnras/advance-article/doi/10.1093/mnras/stae2237/7797286
TI - Discovery of Perun (G329.9-0.5): A New, Young, Galactic SNR
T2 - Monthly Notices of the Royal Astronomical Society
AU - Smeaton, Zachary J.
AU - Filipović, Miroslav D.
AU - Filipović, M. D.
AU - Lazarević, Sanja
AU - Alsaberi, R. Z. E.
AU - Ahmad, Adeel
AU - Araya, M.
AU - Ball, Brianna D
AU - Bordiu, C.
AU - Buemi, Carla S.
AU - Buemi, C.
AU - Bufano, Filomena
AU - Dai, S.
AU - Haberl, Frank
AU - Hopkins, Andrew M
AU - Hopkins, Andrew
AU - Ingallinera, Adriano
AU - Jarrett, Thomas
AU - Jarrett, T. H.
AU - Koribalski, Bärbel S
AU - Koribalski, B.
AU - Kothes, Roland
AU - Kraan-Korteweg, Renée C.
AU - Kraan-Korteweg, R. C.
AU - Leahy, Denis
AU - Leahy, D. A.
AU - Lundqvist, Peter
AU - Maitra, Chandreyee
AU - Martin, Pierrick
AU - Payne, J L
AU - Rowell, Gavin
AU - Rowell, G. P.
AU - Sano, Hidetoshi
AU - Sasaki, M.
AU - Soria, Roberto
AU - Steyn, Nadia
AU - Umana, Grazia
AU - Umana, G.
AU - Urošević, Dejan
AU - Urošević, D.
AU - Velović, Velibor
AU - Vernstrom, T.
AU - Vukotić, Branislav
AU - Vukotić, B.
AU - West, J. L.
PY - 2024
DA - 2024/09/30
PB - Oxford University Press
SP - 2918-2937
IS - 3
VL - 534
SN - 0035-8711
SN - 1365-2966
SN - 1365-8711
ER -
BibTex |
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BibTex (up to 50 authors) Copy
@article{2024_Smeaton,
author = {Zachary J. Smeaton and Miroslav D. Filipović and M. D. Filipović and Sanja Lazarević and R. Z. E. Alsaberi and Adeel Ahmad and M. Araya and Brianna D Ball and C. Bordiu and Carla S. Buemi and C. Buemi and Filomena Bufano and S. Dai and Frank Haberl and Andrew M Hopkins and Andrew Hopkins and Adriano Ingallinera and Thomas Jarrett and T. H. Jarrett and Bärbel S Koribalski and B. Koribalski and Roland Kothes and Renée C. Kraan-Korteweg and R. C. Kraan-Korteweg and Denis Leahy and D. A. Leahy and Peter Lundqvist and Chandreyee Maitra and Pierrick Martin and J L Payne and Gavin Rowell and G. P. Rowell and Hidetoshi Sano and M. Sasaki and Roberto Soria and Nadia Steyn and Grazia Umana and G. Umana and Dejan Urošević and D. Urošević and Velibor Velović and T. Vernstrom and Branislav Vukotić and B. Vukotić and J. L. West and others},
title = {Discovery of Perun (G329.9-0.5): A New, Young, Galactic SNR},
journal = {Monthly Notices of the Royal Astronomical Society},
year = {2024},
volume = {534},
publisher = {Oxford University Press},
month = {sep},
url = {https://academic.oup.com/mnras/advance-article/doi/10.1093/mnras/stae2237/7797286},
number = {3},
pages = {2918--2937},
doi = {10.1093/mnras/stae2237}
}
MLA
Cite this
MLA Copy
Smeaton, Zachary J., et al. “Discovery of Perun (G329.9-0.5): A New, Young, Galactic SNR.” Monthly Notices of the Royal Astronomical Society, vol. 534, no. 3, Sep. 2024, pp. 2918-2937. https://academic.oup.com/mnras/advance-article/doi/10.1093/mnras/stae2237/7797286.