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Journals / Turkish Journal of Physics / 2018 / Cilt: 42 - Sayı: 4

Mapping heavy elements in the supernova remnant G290.1-0.8

Murat HÜDAVERDİ
Pages
415–424
Publication Date
2018-08-15
DOI
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AI Summary & Key Takeaways

AI Insight
⚡ TL;DR(Too Long; Didn't Read)

The EW maps are enhanced in the direction of the X-ray elongation, suggesting that the distorted X-ray structure is dominated by a core-collapse 20∼25 M⊙ progenitor star ejecta.

📌 3 Key Takeaways

🎯
Objective & Hypothesis:We present the imaging and spectroscopic study results of G290.1-0.8 Supernova Remnant (SNR) using the Suzaku X-ray archival data.
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Key Findings & Data:The X-ray spectra is well defined with isothermal plasma of kTe ∼ 0:5 keV.
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Conclusion & Impact:The EW maps are enhanced in the direction of the X-ray elongation, suggesting that the distorted X-ray structure is dominated by a core-collapse 20∼25 M⊙ progenitor star ejecta.
🔬Design:Research Article
📍Scope:Comprehensive Sample
⚙️Variables:Supernova remnants · X-rays · gamma-rays

Abstract

We present the imaging and spectroscopic study results of G290.1-0.8 Supernova Remnant (SNR) using the Suzaku X-ray archival data. The SNR belongs to the mixed-morphology class with its centrally peaked asymmetric X-ray core and distorted radio shell-like plasma. The X-ray spectra is well defined with isothermal plasma of kTe ∼ 0:5 keV. The radial profile shows enhanced elemental abundances. The EW maps reveal inhomogeneous asymmetric spatial distribution of elemental abundances. The northeast of the SNR is bright in Ne, Mg, and Si. The EW maps are enhanced in the direction of the X-ray elongation, suggesting that the distorted X-ray structure is dominated by a core-collapse 20∼25 M⊙ progenitor star ejecta.

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Cite This Article

HÜDAVERDİ, M. (2018). Mapping heavy elements in the supernova remnant G290.1-0.8. Turkish Journal of Physics, Cilt: 42 - Sayı: 4, 415–424. https://ajindex.com/articles/723875

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