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- 爆炸后的影響可以在一種被稱(chēng)為黑洞候選體的X射線(xiàn)雙星中觀(guān)察到。The after-effects are observed in some X-ray binaries known as black hole candidates.
- 他們認為,一個(gè)已知的毫秒脈沖星與一個(gè)已知的X射線(xiàn)雙星之間的這種相似性,為我們提示了這兩類(lèi)天體間長(cháng)期未知的內在聯(lián)系。They suggest that these similarities between a known millisecond pulsar and a known X-ray binary provide the long-sought link between these types of objects.
- X射線(xiàn)雙星X-ray Binaries
- X射線(xiàn)雙星binary X-ray source
- 低質(zhì)量X射線(xiàn)雙星中QPO現象的理論解釋The Theory of Quasi-periodic Oscillation in Low-mass X-ray Binaries
- 對肺部作X射線(xiàn)攝影to sciagraph the lung
- 起源于吸積X射線(xiàn)雙星的中子星,通過(guò)從伴星吸積物質(zhì)而加速到毫秒周期;a recycled neutron star previously in an accreting X-ray binary system which accretes for a long time from a surrounding keplerian disk and spun up to millisecond period.
- 婦產(chǎn)科X射線(xiàn)檢查X-ray examination in gynecology and obstetrics
- 射線(xiàn)雙星就這樣形成了,于是這顆中子星就向成為毫秒脈沖星邁出了關(guān)鍵的第二步。An X-ray binary system has been formed, and the neutron star has made the crucial second step toward becoming a millisecond pulsar.
- X射線(xiàn)CTX-my CT
- X射線(xiàn)光子X-ray photon
- X射線(xiàn)光學(xué)X-ray optics
- X射線(xiàn)造影X-ray angiography
- x射線(xiàn)衍射顯微術(shù)x ray diffraction microscopy
- X射線(xiàn)天文學(xué)X-ray astronomy
- X射線(xiàn)毛細管X-ray capillary
- 多數天文家接受這個(gè)假想的模式,因為他們已經(jīng)在X射線(xiàn)雙星系統中觀(guān)測到了中子星的加速現象,而且幾乎所有的毫秒脈沖星都被發(fā)現時(shí)處于雙星系統中。Most astronomers accept the binary spin-up scenario for creating millisecond pulsars because they have observed neutron stars speeding up in X-ray binary systems, and almost all radio millisecond pulsars are observed to be in binary systems.
- 數字X射線(xiàn)機digiter X-ray machine
- X射線(xiàn)探測器X ray detector
- 分析1985年EXOSAT衛星對銀河核球X射線(xiàn)源GX9+1的觀(guān)測數據,發(fā)現該源存在幾百秒量級的振蕩現象,這一結果有助于了解小質(zhì)量X射線(xiàn)雙星Gx9+1的吸積特性和軌道運動(dòng)。We analyze the Exosat data of the,Galactic bulge source GX9+1 and find it exhibiting some oscillation phenomena in 1985 with a time scale of a few hundred seconds. Our study will contribute to a better understanding of the accretion and orbital properties of this bright low-mass X-ray binary.