The updated orbital ephemeris of high mass X-ray binary Cyg X-3 detected from monitoring X-ray telescopes
碩士 === 國立中央大學 === 天文研究所 === 106 === Cyg X-3 is a high-mass X-ray binary system composed by a Wolf-Rayet star and a compact object. Its 4.8 hr orbital modulation profile is caused by the strong stellar wind from companion with a specific form. We analyzed the light curve collected by the all sky moni...
| Main Authors: | , |
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| Other Authors: | |
| Format: | Others |
| Language: | zh-TW |
| Published: |
2017
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| Online Access: | http://ndltd.ncl.edu.tw/handle/4eunye |