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英語(yǔ)人>網(wǎng)絡(luò)例句>Pulsar 相關(guān)的網(wǎng)絡(luò)例句
Pulsar相關(guān)的網(wǎng)絡(luò)例句
與 Pulsar 相關(guān)的網(wǎng)絡(luò)例句 [注:此內(nèi)容來(lái)源于網(wǎng)絡(luò)免费在线日本视频,僅供參考]

Analysis of ASCA observation of the X-ray pulsar 1SAX J1324.4-6200, we get precise pulse period, and find that it is significantly larger than the pulse period determined from previous observations, agreed well with a linear spin-down of the pulsar.

對(duì)X射線脈沖星1SAX J1324.4-6200的ASCA觀測(cè)作了分析95香蕉视频,獲得其準(zhǔn)確的脈沖周期及周期的演化wwwaaa827com,指出它可能是一低質(zhì)量X射線雙星系統(tǒng)岛国艹在线。

The correlation between short period and weak magnetic field of binary pulsar and millisecond pulsar implies that these pulsars are the recycled pulsars of existing binary accretion process.

雙星脈沖星和毫秒脈沖星的短周期和弱磁場(chǎng)相關(guān)性暗示這些脈沖星是存在雙星吸積過(guò)程的反加速脈沖星性爱黄色视频A片。

The Crab Nebula spans about 10 light-years. In the nebula's very center lies a pulsar: a neutron star as massive as the Sun but with only the size of a small town. The Crab Pulsar rotates about 30 times each second

整個(gè)蟹狀星云跨越約10光年,在其正中心存在一脈沖星---有太陽(yáng)一樣的質(zhì)量但體積只有小鎮(zhèn)大小的中子星国产精品无码无片在线播放,蟹狀星云脈沖星的自轉(zhuǎn)速度約為30圈每秒黄色片黄色网站黄色片。

A pulsar is a celestial object that emits light in short burst a pulsar in the crab nebula flashes at a rate of 30 times/s,suppose the light pulses are caused by the rotation of a spherical object that emits light from a pair of diametrically opposed "flashlights" on its equator.

脈沖星是一種以短爆發(fā)形式輻射光的天體。假設(shè)球型天體赤道面上有一對(duì)"發(fā)光塔"91日韩作爱视频免费观看?,并且這對(duì)發(fā)光塔的聯(lián)線構(gòu)成赤道面的直徑美女视频黄软件,進(jìn)一步假設(shè)光脈沖產(chǎn)生于球形天體的轉(zhuǎn)動(dòng),那么巨蟹座星云中的一個(gè)脈沖星的閃光頻率是每秒30次精品一区综合。

In § 2.3 we study the effects of the oblateness, caused by pulsar rotation, on the pulsar properties, then we calculate the some properties of the pulsar in SN1987A.

即然認(rèn)為這顆光學(xué)脈沖星是老年中子星,要通過(guò)吸積加速使它的自轉(zhuǎn)周期減小到現(xiàn)在的0.5毫秒国产xxxx在线播放,則表面磁場(chǎng)不能超過(guò)2×10〓G老女老肥熟国产在线视频。

Pulsar B is an oddity, in that it is very different from a 'normal' pulsar.

脈沖星B比較怪,與"正常"的脈沖星很不同午夜免费性爱视频。

If the pulsar is old pulsar, its magnetic field will be smaller than 2×10〓G.

如果認(rèn)為這就是自轉(zhuǎn)周期日韩美图精品自拍视频在线观看,則會(huì)對(duì)脈沖星的表面磁場(chǎng)有很強(qiáng)的限制。

This default state after a PULSAR reset is unknown.

PULSAR 復(fù)位后的缺省狀態(tài)是不可知的无码99riav片。

The treatment to pulsar signal only confine to the adding of the pulsar signal by cycles at present.

目前對(duì)脈沖星信號(hào)的處理僅局限于對(duì)脈沖星信號(hào)不同周期的迭加中老妇女毛片黄片视频。

Since the first discovery of pulsar in 1967, static dipole field has been used for a long time to represent pulsar magnetic field in the study of rotating vector model, which is used to interpret the variation of linear polarization position angle with pulse phase.

1967年發(fā)現(xiàn)第一顆脈沖星以來(lái)九九99视频网,在用于解釋線偏振位置角隨脈沖相位變化曲線的旋轉(zhuǎn)矢量模型中,脈沖星磁場(chǎng)通常被近似為靜態(tài)磁偶極場(chǎng)91福利在线播放。

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