How does the stellar wind influence the radio morphology of a supernova remnant
作者： W. W. Tian , M. F. Zhang , D. Wu
关键词:
摘要: We simulate the evolutions of stellar wind and supernova remnant (SNR) originating from a runaway massive star in an uniform Galactic environment based on three-dimensional magnetohydrodynamics models. Taking into consideration, we can explain radio morphologies many remnants. The directions kinematic velocity progenitor, magnetic field line sight are most important factors influencing morphologies. If is perpendicular to field, simulation will give us two different unilateral SNRs bilateral symmetric SNR. parallel obtain asymmetric SNR quasi-circular Our simulations show plays key role evolution SNR, which implies global density distribution play secondary shaping
arxiv.org
sci-hub.st 参考文章(56)
A. J. van Marle, N. L. J. Cox, L. Decin, Eyes in the sky: Interactions between AGB winds and the interstellar magnetic field arXiv: Solar and Stellar Astrophysics. ,(2014) , 10.1051/0004-6361/201424452
E. Matias Schneiter, Eduardo De La Fuente, Pablo F. Velázquez, Simulated X-ray emission from a single-explosion model for a supernova remnant 3C 400.2 Monthly Notices of the Royal Astronomical Society. ,vol. 371, pp. 369- 374 ,(2006) , 10.1111/J.1365-2966.2006.10652.X
Stanley P. Owocki, Bob van Veelen, Nathan Smith, Allard Jan van Marle, Allard Jan van Marle, Numerical models of collisions between core-collapse supernovae and circumstellar shells Monthly Notices of the Royal Astronomical Society. ,vol. 407, pp. 2305- 2327 ,(2010) , 10.1111/J.1365-2966.2010.16851.X
D. M.-A. Meyer, N. Langer, J. Mackey, P. F. Velázquez, A. Gusdorf, Asymmetric supernova remnants generated by Galactic, massive runaway stars Monthly Notices of the Royal Astronomical Society. ,vol. 450, pp. 3080- 3100 ,(2015) , 10.1093/MNRAS/STV898
Allard Jan van Marle, Zakaria Meliani, Alexandre Marcowith, Shape and evolution of wind-blown bubbles of massive stars: on the effect of the interstellar magnetic field arXiv: Solar and Stellar Astrophysics. ,(2015) , 10.1051/0004-6361/201425230
V. V. Gvaramadze, K. M. Menten, A. Y. Kniazev, N. Langer, J. Mackey, A. Kraus, D. M.-A. Meyer, T. Kamiński, IRC 10414: a bow-shock-producing red supergiant star ⋆ Monthly Notices of the Royal Astronomical Society. ,vol. 437, pp. 843- 856 ,(2014) , 10.1093/MNRAS/STT1943
William W. Craig, Charles J. Hailey, Ryszard L. Pisarski, ROSAT Observations of the Supernova Remnant CTB 1 The Astrophysical Journal. ,vol. 488, pp. 307- 316 ,(1997) , 10.1086/304666
P. Brian Cameron, Kazimierz J. Borkowski, Jeonghee Rho, Jeonghee Rho, Thomas G. Pannuti, Thomas G. Pannuti, Thomas G. Pannuti, MIXED-MORPHOLOGY SUPERNOVA REMNANTS IN X-RAYS: ISOTHERMAL PLASMA IN HB21 AND PROBABLE OXYGEN-RICH EJECTA IN CTB 1 The Astronomical Journal. ,vol. 140, pp. 1787- 1805 ,(2010) , 10.1088/0004-6256/140/6/1787
Katsuji Koyama, Shigeo Yamauchi, Aya Bamba, Masaru Ueno, A Diffuse X-Ray Source, AX J1843.80352: Association with the Radio Complex G28.6-0.1 and Identification of a New Supernova Remnant Publications of the Astronomical Society of Japan. ,vol. 53, ,(2001) , 10.1093/PASJ/53.4.L21
O. Petruk, V. Beshley, F. Bocchino, S. Orlando, Some properties of synchrotron radio and inverse-Compton gamma-ray images of supernova remnants Monthly Notices of the Royal Astronomical Society. ,vol. 395, pp. 1467- 1475 ,(2009) , 10.1111/J.1365-2966.2009.14563.X