Orbital and spin parameter evolutions of high mass X-ray binary of LMC X-4
碩士 === 國立中央大學 === 天文研究所 === 105 === LMC X-4 is a high-mass eclipsing X-ray binary consisting of an early type star and a neutron star as an accretor. The orbital period of the binary is 1.4 days. The pulsation period of neutron star is 13.5 $s$. It also has a superorbital modulation of period of 30....
| Main Authors: | , |
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| Other Authors: | |
| Format: | Others |
| Language: | zh-TW |
| Published: |
2016
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| Online Access: | http://ndltd.ncl.edu.tw/handle/dgwaar |