Theoretical Study of Gamma-ray Pulsars
We use the non-stationary three dimensional two-layer outer gap model to explain gamma-ray emissions from a pulsar magnetosphere. We found out that for some pulsars like the Geminga pulsar, it was hard to explain emissions above a level of around 1 GeV. We then developed the model into a non-stati...
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| Principais autores: | , |
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| Formato: | Artigo |
| Idioma: | Inglês |
| Publicado em: |
The Korean Space Science Society
2016-06-01
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| coleção: | Journal of Astronomy and Space Sciences |
| Assuntos: | |
| Acesso em linha: | http://ocean.kisti.re.kr/downfile/volume/kosss/OJOOBS/2016/v33n2/OJOOBS_2016_v33n2_69.pdf |
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