Modelling gamma-ray light curves of phase-aligned millisecond pulsars
Author:
Affiliation:
1. Department of Astronomy, Key Laboratory of Astroparticle Physics of Yunnan Province, Yunnan University, Kunming 650091, China
Funder
Natural Science Foundation of China
Top Talents Program of Yunnan Province
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/475/2/2185/23734278/stx3322.pdf
Reference43 articles.
1. Detection of 16 Gamma-Ray Pulsars Through Blind Frequency Searches Using the Fermi LAT
2. THE FIRST FERMI LARGE AREA TELESCOPE CATALOG OF GAMMA-RAY PULSARS
3. THE SECOND FERMI LARGE AREA TELESCOPE CATALOG OF GAMMA-RAY PULSARS
4. A millisecond pulsar
5. UNCERTAINTIES OF MODELING GAMMA-RAY PULSAR LIGHT CURVES USING VACUUM DIPOLE MAGNETIC FIELD
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1. Trajectories and radiation of charged particles in the pulsar magnetosphere;Monthly Notices of the Royal Astronomical Society;2022-04-07
2. The Emission Physics of Millisecond Pulsars;Astrophysics and Space Science Library;2021-11-26
3. Modelling pulsed gamma-ray emissions from millisecond pulsars with double peaks;Monthly Notices of the Royal Astronomical Society;2019-07-30
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