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Gamma-ray emission from millisecond pulsars - an Outergap perspective

In this review paper we explain the following gamma-ray emission features from the millisecond pulsars. (1) Why is the dipolar field of millisecond pulsars so weak but the magnetic pair creation process may still be able to control the size of the outergap? (2) A sub-GeV pulse component could occu...

Deskribapen osoa

Gorde:
Xehetasun bibliografikoak
Egile nagusia: Kwong Sang Cheng
Formatua: Artigo
Hizkuntza:Inglês
Argitaratua: The Korean Space Science Society 2013-09-01
Saila:Journal of Astronomy and Space Sciences
Gaiak:
Sarrera elektronikoa:http://ocean.kisti.re.kr/downfile/volume/kosss/OJOOBS/2013/v30n3/OJOOBS_2013_v30n3_153.pdf
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