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Numerical simulations of mass loading in the tails of bow-shock pulsar-wind nebulae

  • Published:2018-09-15 Issue:3 Volume:481 Page:3394-3400
  • ISSN:0035-8711
  • Container-title:Monthly Notices of the Royal Astronomical Society
  • language:en
  • Short-container-title:

Author:

Olmi B123,Bucciantini N123,Morlino G24ORCID

Affiliation:

1. Dipartimento di Fisica e Astronomia, Università degli Studi di Firenze, Via G. Sansone 1, I-50019 Sesto F. no, Italy

2. INAF - Osservatorio Astrofisico di Arcetri, Largo E. Fermi 5, I-50125 Firenze, Italy

3. INFN - Sezione di Firenze, Via G. Sansone 1, I-50019 Sesto F. no, Italy

4. Gran Sasso Science Institute, Viale Francesco Crispi 7, I-67100 L’Aquila, Italy

Funder

Ministero dell’Istruzione, dell’Università e della Ricerca

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Cited by 6 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. The nature of the X-ray filaments around bow shock pulsar wind nebulae;Astronomy & Astrophysics;2024-03-28

2. Evolved Pulsar Wind Nebulae;Universe;2023-09-01

3. The Dawes Review 11: From young to old: The evolutionary path of Pulsar Wind Nebulae;Publications of the Astronomical Society of Australia;2023

4. Fast-moving pulsars as probes of interstellar medium;Monthly Notices of the Royal Astronomical Society;2020-06-08

5. Full-3D relativistic MHD simulations of bow shock pulsar wind nebulae: emission and polarization;Monthly Notices of the Royal Astronomical Society;2019-07-30
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