Determining the evolutionary status of supernova remnants-Reference-Cited by-同舟云学术

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Determining the evolutionary status of supernova remnants

Published:2020-09-23 Issue:10 Volume:4 Page:910-912
ISSN:2397-3366
Container-title:Nature Astronomy
language:en
Short-container-title:Nat Astron

Author:

Urošević Dejan^ORCID

Publisher

Springer Science and Business Media LLC

Subject

Astronomy and Astrophysics

Link

https://www.nature.com/articles/s41550-020-01228-5.pdf

Reference16 articles.

1. Shklovskii, I. S. Astron. Zh. 37, 256–262 (1960).

2. Shklovskii, I. S. Astron. Zh. 37, 369–378 (1960).

3. Urošević, D. Astrophys. Space Sci. 354, 541–552 (2014).

4. Pacholczyk, A. G. Radio Astrophysics: Nonthermal Processes in Galactic and Extragalactic Sources (Freeman, 1970).

5. Pavlović, M. Z. et al. Astrophys. J. 852, 84 (2018).

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1. Radio continuum study of the Large Magellanic Cloud supernova remnant Honeycomb Nebula;Serbian Astronomical Journal;2024

2. ATCA study of Small Magellanic Cloud supernova remnant 1E 0102.2–7219;Monthly Notices of the Royal Astronomical Society;2023-10-27

3. EMU Detection of a Large and Low Surface Brightness Galactic SNR G288.8–6.3;The Astronomical Journal;2023-09-07

4. SRG/eROSITA discovery of a radio-faint X-ray candidate supernova remnant SRGe J003602.3+605421 = G121.1−1.9;Monthly Notices of the Royal Astronomical Society;2023-03-20

5. Deep X-Ray and Radio Observations of the First Outburst of the Young Magnetar Swift J1818.0−1607;The Astrophysical Journal;2023-01-01

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