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Süpernova Kalıntısı G12.8-0.0’nin Suzaku ile X-ışın Dalgaboylarında Araştırılması

Yıl 2022, Sayı: 35, 464 - 468, 07.05.2022
https://doi.org/10.31590/ejosat.1083773

Öz

Galaksimizde bulunan G12.8-0.0, merkezinde pulsar PSR J1813–1749’u barındıran bir kompozit süpernova kalıntısıdır (SNK). Bu çalışmada, yüksek tayfsal çözünürlüklü Suzaku verisi kullanılarak, SNK’dan gelen ışımanın X-ışın doğası ve tayfsal özellikleri araştırılmıştır. X-ışın tayfı ısısal olmayan bir model ile (foton indeksi Γ ∼ 1.97) iyi tanımlanmaktadır ve yüksek soğurma sütun yoğunluğuna (NH ∼12.1x1022 cm-2) sahiptir. Ayrıca, bu çalışmada gelecek nesil X-ışın uyduları olan XRISM ve Athena simülasyonları da sunulmuştur. Her iki simülasyonda da ısısal ışımadan gelen Mg ve Si çizgi salmaları açıkça görülmüştür ve bu da kalıntıda hala süpernova patlamasının izleri olduğunu gösterir.

Destekleyen Kurum

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Proje Numarası

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Teşekkür

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Kaynakça

  • Arnaud, K. A. (1996), in Jacoby G., Barnes J., eds, ASP Conf. Ser. Vol. 101, Astronomical data analysis software and systems V. Astron. Soc. Pac. 101, 17-20.
  • Barret, D., Cucchetti, E. (2018). X-IFU response matrices [online]. Website http://x-ifu-resources.irap.omp.eu/.
  • Brogan, C. L., Gaensler, B. M., Gelfand, J. D., Lazendic, J. S., Lazio, T. J., Kassim, N. E., & McClure-Griffiths, N. M. (2005). Discovery of a Radio Supernova Remnant and Nonthermal X-Rays Coincident with the TeV Source HESS J1813-178. The Astrophysical Journal, 629, L105-L108. doi: 10.1086/491471.
  • Dzib, S. A., Rodriguez, L. F., Karuppusamy, R., Loinard, L., Medina, S.-N. X. (2018). The Enigmatic Compact Radio Source Coincident with the Energetic X-Ray Pulsar PSR J1813-1749 and HESS J1813-178. The Astrophysical Journal, 866, 100. doi: 10.3847/1538-4357/aada07.
  • Funk, S. et al. (2007). XMM-Newton observations of HESS J1813-178 reveal a composite Supernova remnant. Astronomy & Astrophysics, 470, 249-257. doi: 10.1051/0004-6361:20066779.
  • Gaensler, B. M., & Slane, P. O. (2006). The Evolution and Structure of Pulsar Wind Nebulae. Annual Review of Astronomy & Astrophysics, 44, 17-47. doi: 10.1146/annurev.astro.44.051905.092528.
  • Green, D. A. (2019). A revised catalogue of 294 Galactic supernova remnants. Journal of Astrophysics and Astronomy, 40, 36. doi: 10.1007/s12036-019-9601-6.
  • Gotthelf, E. V., & Halpern, J. P. (2009). Discovery of a Highly Energetic X-Ray Pulsar Powering HESS J1813-178 in the Young Supernova Remnant G12.82-0.02. The Astrophysical Journal Letters, 700, L158-L161. doi: 10.1088/0004-637X/700/2/L158.
  • Helfand, D. J. et al. (2007). Discovery of the Putative Pulsar and Wind Nebula Associated with the TeV Gamma-Ray Source HESS J1813-178. The Astrophysical Journal, 665, 1297-1303. doi: 10.1086/519734.
  • Ishisaki, Y., Maeda, Y., Fujimoto, R. et al. (2007). Monte Carlo simulator and ancillary response generator of Suzaku XRT/XIS system for spatially extended source analysis. Publications of the Astronomical Society of Japan, 59, 113-132. doi: 10.1093/pasj/59.sp1.S113.
  • Ishisaki, Y., Ezoe, Y., Yamada, S., et al. (2018). Resolve Instrument on X-ray Astronomy Recovery Mission (XARM). Journal of Low Temperature Physics, 193, 991–995.
  • Koyama, K. et al. (2007). X-Ray Imaging Spectrometer (XIS) on Board Suzaku. Publications of the Astronomical Society of Japan, 59, 23-33. doi: 10.1093/pasj/59.sp1.S23.
  • Messineo, M., Davies, B., Figer, D. F., Kudritzki, R. P., Valenti, E., Trombley, C., Najarro, F., Rich, R. M. (2011). Massive Stars in the Cl 1813-178 Cluster: An Episode of Massive Star Formation in the W33 Complex. The Astrophysical Journal, 733, 41. doi: 10.1088/0004-637X/733/1/41.
  • Mitsuda, K., et al. (2007). The X-Ray Observatory Suzaku. Publications of the Astronomical Society of Japan, 59, S1-S7. doi: 10.1093/pasj/59.sp1.S1. Nandra, K., Barret, D., Barcons, X., et al. (2013). The hot and energetic universe: A white paper presenting the science theme motivating the Athena+ mission. Athena mission proposal, arXiv:1306.2307.
  • Pajot, F., Lam Trong, T., den Herder, J.-W., Piro, L., & Cappi, M. (2018). The Athena X-ray integral field unit (X-IFU). Journal of Low Temperature Physics, 193, 901-907.
  • Rho, J., Petre, R. (1998). Mixed-Morphology Supernova Remnants. The Astrophysical Journal Letters, 503, L167-L170. doi: 10.1086/311538.
  • Tashiro, M. et al. (2018), in Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Series, Vol. 10699, Proc. SPIE, 1069922.
  • Tawa, N., Hayashida, K., Nagai, M. et al. (2008). Reproducibility of non-X-Ray background for the X-Ray imaging spectrometer aboard Suzaku. Publications of the Astronomical Society of Japan, 60, S11-S24. doi: 10.1093/pasj/60.sp1.S11.
  • Ubertini, P. (2005). INTEGRAL IGR J18135-1751 = HESS J1813-178: A New Cosmic High-Energy Accelerator from keV to TeV Energies. The Astrophysical Journal, 629, L109-L112. doi: 10.1086/447766.
  • Vink, J. (2012). Supernova remnants: the X-ray perspective. The Astronomy and Astrophysics Review, 20, 49. doi: 10.1007/s00159-011-0049-1.
  • Vink, J. (2020). Physics and Evolution of Supernova Remnants. Cham, Switzerland: Springer International Publishing.
  • Wilms, J., Allen, A., McCray, R. (2000). On the absorption of X-rays in the interstellar medium. The Astrophysical Journal, 542, 914-924. doi: 10.1086/317016.
  • Woosley, S. & Janka, T. (2005). The physics of core-collapse supernovae. Nature Physics, 1, 147–154. doi: 10.1038/nphys172.
  • Wynn, C. G. Ho, et al. (2020). Proper motion, spectra, and timing of PSR J1813–1749 using Chandra and NICER. Monthly Notices of the Royal Astronomical Society, 498, 4396–4403. doi: 10.1093/mnras/staa2653.
  • XRISM Science Team 2020, Science with the X-ray Imaging and Spectroscopy Mission (XRISM). arXiv e-prints, p. arXiv:2003.04962.

X-ray Investigation of Supernova Remnant G12.8-0.0 with Suzaku

Yıl 2022, Sayı: 35, 464 - 468, 07.05.2022
https://doi.org/10.31590/ejosat.1083773

Öz

The Galactic supernova remnant (SNR) G12.8-0.0 is a member of the class of composite SNRs and hosts the pulsar PSR J1813–1749. In this work, we investigate the X-ray nature of the emission and spectral parameters of the SNR using the high spectral resolution data from Suzaku. We found that the X-ray spectrum of G12.8-0.0 can be fitted by a non-thermal model with a high absorbing column density of NH ∼12.1x1022 cm-2 and a photon index of Γ ∼ 1.97. We also present spectral simulations of G12.8-0.0 for the future missions, XRISM and Athena. The thermal emission lines of Mg and Si are clearly resolved in both simulated spectra, indicating the presence of ejecta.

Proje Numarası

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Kaynakça

  • Arnaud, K. A. (1996), in Jacoby G., Barnes J., eds, ASP Conf. Ser. Vol. 101, Astronomical data analysis software and systems V. Astron. Soc. Pac. 101, 17-20.
  • Barret, D., Cucchetti, E. (2018). X-IFU response matrices [online]. Website http://x-ifu-resources.irap.omp.eu/.
  • Brogan, C. L., Gaensler, B. M., Gelfand, J. D., Lazendic, J. S., Lazio, T. J., Kassim, N. E., & McClure-Griffiths, N. M. (2005). Discovery of a Radio Supernova Remnant and Nonthermal X-Rays Coincident with the TeV Source HESS J1813-178. The Astrophysical Journal, 629, L105-L108. doi: 10.1086/491471.
  • Dzib, S. A., Rodriguez, L. F., Karuppusamy, R., Loinard, L., Medina, S.-N. X. (2018). The Enigmatic Compact Radio Source Coincident with the Energetic X-Ray Pulsar PSR J1813-1749 and HESS J1813-178. The Astrophysical Journal, 866, 100. doi: 10.3847/1538-4357/aada07.
  • Funk, S. et al. (2007). XMM-Newton observations of HESS J1813-178 reveal a composite Supernova remnant. Astronomy & Astrophysics, 470, 249-257. doi: 10.1051/0004-6361:20066779.
  • Gaensler, B. M., & Slane, P. O. (2006). The Evolution and Structure of Pulsar Wind Nebulae. Annual Review of Astronomy & Astrophysics, 44, 17-47. doi: 10.1146/annurev.astro.44.051905.092528.
  • Green, D. A. (2019). A revised catalogue of 294 Galactic supernova remnants. Journal of Astrophysics and Astronomy, 40, 36. doi: 10.1007/s12036-019-9601-6.
  • Gotthelf, E. V., & Halpern, J. P. (2009). Discovery of a Highly Energetic X-Ray Pulsar Powering HESS J1813-178 in the Young Supernova Remnant G12.82-0.02. The Astrophysical Journal Letters, 700, L158-L161. doi: 10.1088/0004-637X/700/2/L158.
  • Helfand, D. J. et al. (2007). Discovery of the Putative Pulsar and Wind Nebula Associated with the TeV Gamma-Ray Source HESS J1813-178. The Astrophysical Journal, 665, 1297-1303. doi: 10.1086/519734.
  • Ishisaki, Y., Maeda, Y., Fujimoto, R. et al. (2007). Monte Carlo simulator and ancillary response generator of Suzaku XRT/XIS system for spatially extended source analysis. Publications of the Astronomical Society of Japan, 59, 113-132. doi: 10.1093/pasj/59.sp1.S113.
  • Ishisaki, Y., Ezoe, Y., Yamada, S., et al. (2018). Resolve Instrument on X-ray Astronomy Recovery Mission (XARM). Journal of Low Temperature Physics, 193, 991–995.
  • Koyama, K. et al. (2007). X-Ray Imaging Spectrometer (XIS) on Board Suzaku. Publications of the Astronomical Society of Japan, 59, 23-33. doi: 10.1093/pasj/59.sp1.S23.
  • Messineo, M., Davies, B., Figer, D. F., Kudritzki, R. P., Valenti, E., Trombley, C., Najarro, F., Rich, R. M. (2011). Massive Stars in the Cl 1813-178 Cluster: An Episode of Massive Star Formation in the W33 Complex. The Astrophysical Journal, 733, 41. doi: 10.1088/0004-637X/733/1/41.
  • Mitsuda, K., et al. (2007). The X-Ray Observatory Suzaku. Publications of the Astronomical Society of Japan, 59, S1-S7. doi: 10.1093/pasj/59.sp1.S1. Nandra, K., Barret, D., Barcons, X., et al. (2013). The hot and energetic universe: A white paper presenting the science theme motivating the Athena+ mission. Athena mission proposal, arXiv:1306.2307.
  • Pajot, F., Lam Trong, T., den Herder, J.-W., Piro, L., & Cappi, M. (2018). The Athena X-ray integral field unit (X-IFU). Journal of Low Temperature Physics, 193, 901-907.
  • Rho, J., Petre, R. (1998). Mixed-Morphology Supernova Remnants. The Astrophysical Journal Letters, 503, L167-L170. doi: 10.1086/311538.
  • Tashiro, M. et al. (2018), in Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Series, Vol. 10699, Proc. SPIE, 1069922.
  • Tawa, N., Hayashida, K., Nagai, M. et al. (2008). Reproducibility of non-X-Ray background for the X-Ray imaging spectrometer aboard Suzaku. Publications of the Astronomical Society of Japan, 60, S11-S24. doi: 10.1093/pasj/60.sp1.S11.
  • Ubertini, P. (2005). INTEGRAL IGR J18135-1751 = HESS J1813-178: A New Cosmic High-Energy Accelerator from keV to TeV Energies. The Astrophysical Journal, 629, L109-L112. doi: 10.1086/447766.
  • Vink, J. (2012). Supernova remnants: the X-ray perspective. The Astronomy and Astrophysics Review, 20, 49. doi: 10.1007/s00159-011-0049-1.
  • Vink, J. (2020). Physics and Evolution of Supernova Remnants. Cham, Switzerland: Springer International Publishing.
  • Wilms, J., Allen, A., McCray, R. (2000). On the absorption of X-rays in the interstellar medium. The Astrophysical Journal, 542, 914-924. doi: 10.1086/317016.
  • Woosley, S. & Janka, T. (2005). The physics of core-collapse supernovae. Nature Physics, 1, 147–154. doi: 10.1038/nphys172.
  • Wynn, C. G. Ho, et al. (2020). Proper motion, spectra, and timing of PSR J1813–1749 using Chandra and NICER. Monthly Notices of the Royal Astronomical Society, 498, 4396–4403. doi: 10.1093/mnras/staa2653.
  • XRISM Science Team 2020, Science with the X-ray Imaging and Spectroscopy Mission (XRISM). arXiv e-prints, p. arXiv:2003.04962.
Toplam 25 adet kaynakça vardır.

Ayrıntılar

Birincil Dil Türkçe
Konular Mühendislik
Bölüm Makaleler
Yazarlar

Cihad Deniz 0000-0002-5996-5814

Aytap Sezer 0000-0002-1396-3282

Proje Numarası -
Yayımlanma Tarihi 7 Mayıs 2022
Yayımlandığı Sayı Yıl 2022 Sayı: 35

Kaynak Göster

APA Deniz, C., & Sezer, A. (2022). Süpernova Kalıntısı G12.8-0.0’nin Suzaku ile X-ışın Dalgaboylarında Araştırılması. Avrupa Bilim Ve Teknoloji Dergisi(35), 464-468. https://doi.org/10.31590/ejosat.1083773