Model Spectra of Surface Thermal Emission from Neutron Stars with Strong Magnetic Fields
碩士 === 國立清華大學 === 物理學系 === 91 === We develop an atmosphere model for neutron stars with strong magnetic fields. The atmosphere is composed of pure hydrogen. We assume it is fully ionized and the opacity considered is contributed from the Thomson scattering and free-free absorption. The e...
| Main Authors: | , |
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| Other Authors: | |
| Format: | Others |
| Language: | zh-TW |
| Published: |
2003
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| Online Access: | http://ndltd.ncl.edu.tw/handle/44268283839356677985 |