A 3D MHD simulation of SN 1006: a polarized emission study for the turbulent case-Reference-Cited by-同舟云学术

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A 3D MHD simulation of SN 1006: a polarized emission study for the turbulent case

Published:2017-01-11 Issue: Volume: Page:stx064
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:Mon. Not. R. Astron. Soc.

Author:

Velázquez P. F.,Schneiter E. M.,Reynoso E. M.,Esquivel A.,De Colle F.,Toledo-Roy J. C.,Gómez D.O.,Sieyra M.V.,Moranchel-Basurto A.

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Cited by 13 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. Survival of the Fittest: Numerical Modeling of SN 2014C;The Astrophysical Journal;2022-05-01

2. 3D MHD simulations of the supernova remnant CTB 109;Monthly Notices of the Royal Astronomical Society;2021-10-11

3. Magneto-hydrodynamic simulations of young supernova remnants and their energy-conversion phase;Monthly Notices of the Royal Astronomical Society;2021-05-10

4. Evolutions of Young Type Ia Supernova Remnants with Two Initial Density Profiles in a Turbulent Medium;The Astrophysical Journal;2021-03-01

5. Non-thermal radio supernova remnants of exiled Wolf–Rayet stars;Monthly Notices of the Royal Astronomical Society;2021-02-17

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