Search for the Rotation Period of the Neutron Star in Scorpius X-1

碩士 === 國立清華大學 === 天文研究所 === 98 === Abstract Scorpius X-1 (Sco X-1) is the brightest extra-solar X-ray source in the sky. We present the result of searches for the neutron star rotation period in the X-ray emission from Sco X-1. Although a rich spectrum of quasi-periodic pulsations has been fo...

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Bibliographic Details
Main Authors: Kao, Kai-Wei, 高凱威
Other Authors: Chang, Hsiang-Kuang
Format: Others
Language:en_US
Published: 2010
Online Access:http://ndltd.ncl.edu.tw/handle/32396356157556285032