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愚石 发表于 2013-6-10 10:52 | 显示全部楼层 |阅读模式 来自: 中国–河北–石家庄–平山县 联通

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这是今天才发布在 arXiv 上的一篇文章:arXiv:1306.1733

标题是 A model for the orbital modulation of PSR J0737-3039B (一个关于脉冲星 PSR J0737-3039B 的轨道调制的模型)。

摘要如下:
A model was constructed to explain the orbit modulation of PSR J0737-3039B (referred to as B), which included the following suppositions: (1) B has arrived at the aged period and generally cannot emit observable light; (2) The PSR J0737-3039A (referred to as A) is dynamic and is encircled by dense charged particles. When A revolves along its orbit, some of the particles are scattered and form a particle cloud band along its orbit; (3) When passing the two intersection points of the orbits, B goes through the cloud band and drives the cloud particles to emit light; (4) Generally, B passes twice through the cloud band every orbit cycle; hence, there are two bright phases along the orbit. (5) It is the complexities of the distribution of the cloud particles and B's emission region that cause the bright phases to drift away from the orbit intersections. We also provide two predictions for the coming performance of B to test our model.

PSR J0737-3039B 的轨道调制提出了一个模型,同时提出了两个预言。
ddding 发表于 2013-6-12 15:27 | 显示全部楼层 来自: 中国–浙江–绍兴 电信
真了不起,加油兄弟!{:soso_e179:}
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ddding 发表于 2013-6-12 15:29 | 显示全部楼层 来自: 中国–浙江–绍兴 电信
Zhu-Xing Liang, Yi Liang,两个作者
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hzg0728 发表于 2013-6-14 00:16 | 显示全部楼层 来自: 中国–广东–广州 移动
祝贺!
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bsese 发表于 2015-6-6 05:21 来自手机 | 显示全部楼层 来自: 中国–浙江–温州–平阳县 电信
祝贺!!!
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taiwayaya 发表于 2015-6-7 10:52 | 显示全部楼层 来自: 中国–辽宁–大连 联通
提示: 作者被禁止或删除 内容自动屏蔽
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