Pulsed γ-ray emission from magnetar 1E 2259+586

Pulsed γ-ray emission from magnetar 1E 2259+586

Anomalous X-ray pulsars (AXPs) are thought to be magnetars which are young isolated neutron stars with extremely strong magnetic fields of >1014 Gauss. Their tremendous magnetic fields inferred from the spin parameters provide a huge energy reservoir to power the observed X-ray emission. High-e...

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Bibliographic Details
Main Authors: Jason Hung Kit Wu, Chung Yue Hui, Regina Hsiu Hui Huang, Albert Kwok Hing Kong, Kwong Sang Cheng, Jumpei Takata, Pak Hin Thomas Tam, Eric Man Ho Wu, Joe Liu
Format: Article
Language:English
Published: Korean Space Science Society (KSSS) 2013-06-01
Series:Journal of Astronomy and Space Sciences
Subjects:
pulsars
gamma-rays
Online Access:http://ocean.kisti.re.kr/downfile/volume/kosss/OJOOBS/2013/v30n2/OJOOBS_2013_v30n2_83.pdf

Internet

http://ocean.kisti.re.kr/downfile/volume/kosss/OJOOBS/2013/v30n2/OJOOBS_2013_v30n2_83.pdf

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