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

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

Murat HÜDAVERDİ
Sayfa
415–424
Yayın Tarihi
2018-08-15
DOI
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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 Maddede Bu Makale

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Amaç & Hipotez: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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Temel Bulgular & Veri:The X-ray spectra is well defined with isothermal plasma of kTe ∼ 0:5 keV.
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Sonuç & Katkı: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.
🔬Tür:Araştırma Makalesi
📍Kapsam:Genişletilmiş Akademik Örneklem
⚙️Değişkenler: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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Bu Makaleye Atıf Yap

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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Kaynakça (22)

  1. Seward, F. D. Comments on Astrophysics 1985, 11, 15-51.
  2. Rho, J.; Petre, R. Astrophys. J. 1998, 503, L167-L170. Slane, P.; Smith, R. K.; Hughes, J. P.; Petre, R. Astrophys. J. 2002, 564, 284-290.
  3. Mills, B. Y.; Slee, O. B.; Hill, E. R. Aust. J. Phys. 1961, 14, 497-507.
  4. Kirshner, R. P.; Winkler, P. F. Jr. Astrophys. J. 1979, 227, 853-855.
  5. Kesteven, M. J.; Caswell, J. L. Astron. Astrophys. 1987, 183, 118-128. Milne D. K.; Caswell J. L.; Kesteven M. J.; Haynes R. F.; Roger R. S. Proceedings of the Astronomical Society of Australia 1989, 8, 187-194.
  6. Reynoso, E. M.; Johnston, S.; Green, A. J.; Koribalski, B. S. Mon. Not. R. Astron. Soc. 2006, 369, 416-424.
  7. Seward, F. D. Astrophys. J. Suppl. S. 1990, 73, 781-819.
  8. Garcia, F.; Combi, J. A.; Albacete-Colombo, J. F.; Romero, G. E.; Bocchino, F.; Lopez-Santiago, J. Astron. Astrophys. 2012, 546, 91-99.
  9. Kamitsukasa, F.; Koyama, K.; Uchida, H.; Nakajima, H.; Hayashida, K.; Mori, K.; Katsuda, S.; Tsunemi, H. Publ. Astron. Soc. Jpn. 2015, 67, 1-8.
  10. Auchettl, K.; Slane, P.; Castro, D.; Foster, A. R.; Smith, R. K. Astrophys. J. 2015, 810, 43, 1-12.
  11. Yamaguchi, H.; Tanaka, M.; Maeda, K.; Slane, P. O.; Foster, A.; Smith, R. K.; Katsuda, S.; Yoshii, R. Astrophys. J. 2012, 749, 137-146.
  12. Atwood, W. B.; Abdo, A. A.; Ackermann, M.; Althouse, W.; Anderson, B.; Axelsson, M.; Baldini, L.; Ballet, J.; Band, D. L.; Barbiellini, G. et al. Astrophys. J. 2009, 697, 1071-1102.
  13. Pavan, L.; Bordas, P.; P￿hlhofer, G.; Filipovic, M. D.; De Horta, A.; O’Brien, A.; Balbo, M.; Walter, R.; Bozzo, E.; Ferrigno, C. et al. Astron. Astrophys. 2014, 562, 122-130.
  14. Auchettl, K.; Ng, C.-Y.; Wong, B. T. T.; Lopez, Laura; Slane, P. Astrophys. J. 2017, 847, 2-20.
  15. Koyama, K.; Hyodo, Y.; Inui, T.; Nakajima, H.; Matsumoto, H.; Tsuru, T. G.; Takahashi, T.; Maeda, Y.; Yamazaki, N. Y.; Murakami, H. et al. Publ. Astron. Soc. Jpn. 2007, 59, 245-255.
  16. Whiteoak, J. B. Z.; Green, A. J. Astron Astrophys 1996, 118, 329-380.
  17. Ishisaki, Y.; Maeda, Y.; Fujimoto, R.; Ozaki, M.; Ebisawa, K.; Takahashi, T.; Ueda, Y.; Ogasaka, Y.; Ptak, A.; Mukai, K. et al. Publ. Astron. Soc. Jpn. 2007, 59, 113-132.
  18. Arnaud, K. A. Astr. Soc. P. 1996, 101, 17-20.
  19. Wilms, J.; Allen, A.; McCray, R. Astrophys. J. 2000, 542, 914-924.
  20. Yasumi, M.; Nobukawa, M.; Nakashima, S.; Uchida, H.; Sugawara, R.; Tsuru, T. G.; Tanaka, T.; Koyama, K. Publ. Astron. Soc. Jpn. 2014, 66, 68-77.
  21. Woosley, S. E.; Weaver, T. A. Astrophys. J. 1995, 101, 181-235.
  22. Sarazin, C. L. X-ray Emi