A laminar model for the magnetic field structure in bow-shock pulsar wind nebulae-Reference-Cited by-同舟云学术

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A laminar model for the magnetic field structure in bow-shock pulsar wind nebulae

Published:2018-05-05 Issue:2 Volume:478 Page:2074-2085
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Bucciantini N¹²³

Affiliation:

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

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

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

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/478/2/2074/25060331/sty1199.pdf

Reference128 articles.

1. An anomalous positron abundance in cosmic rays with energies 1.5–100 GeV

2. Measurement of the flux of primary cosmic ray antiprotons with energies of 60 MeV to 350 GeV in the PAMELA experiment

3. First Result from the Alpha Magnetic Spectrometer on the International Space Station: Precision Measurement of the Positron Fraction in Primary Cosmic Rays of 0.5–350 GeV

4. Magnetic field and plasma flow structure near the magnetopause

5. Pair formation above pulsar polar caps - Structure of the low altitude acceleration zone

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1. Pulsar Wind Nebulae;Handbook of X-ray and Gamma-ray Astrophysics;2024

2. On the plerionic rectangular supernova remnants of static progenitors;Monthly Notices of the Royal Astronomical Society;2023-11-15

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

4. Resolving the Bow Shock and Tail of the Cannonball Pulsar PSR J0002+6216;The Astrophysical Journal;2023-03-01

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

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