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)作了分析永久免费观看的毛片app，獲得其準(zhǔn)確的脈沖周期及周期的演化91po精品国产，指出它可能是一低質(zhì)量X射線雙星系統(tǒng)网站网站AA片。

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程的反加速脈沖星。

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光年欧美永久精品，在其正中心存在一脈沖星---有太陽一樣的質(zhì)量但體積只有小鎮(zhèn)大小的中子星网禁呦视频在线播放www，蟹狀星云脈沖星的自轉(zhuǎn)速度約為30圈每秒。

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)形式輻射光的天體亚洲最黄视频。假設(shè)球型天體赤道面上有一對(duì)"發(fā)光塔"人人操久久，并且這對(duì)發(fā)光塔的聯(lián)線構(gòu)成赤道面的直徑，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次免费看日本黄色视频。

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亚洲欧美日韩精品视频一区，要通過吸積加速使它的自轉(zhuǎn)周期減小到現(xiàn)在的0.5毫秒国产永久免费看高清视频，則表面磁場(chǎng)不能超過2×10〓G两女同互玩丝袜脚一区二区。

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"的脈沖星很不同亚洲综合乱伦。

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)周期亚洲高清不卡A片一区二区三区，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3p性A片免费。

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)不同周期的迭加国产又黄又粗又湿视频免费观看。

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，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www.luanlunshipin，脈沖星磁場(chǎng)通常被近似為靜態(tài)磁偶極場(chǎng)黄色视频在线观看免费www。