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- sdark GRBs 暗暴
- A correlation between PFP and GrB was found. PFP与GrB的表达具有相关性。
- The study in my thesis focuses on the GRB afterglows. 本论文的研究集中在伽玛暴的余辉方面。
- The oddball GRB is visible in the center of the right image. 这奇怪的GRB在右部图像的中心是可见的。
- On September 16, 2008, Fermi picked up the most powerful GRB observed to date. 2008年9月16日，费米望远镜发现了迄今为止最为强烈的伽马射线爆发。
- Until recently, the largest red shift ever measured for a GRB was 6.3. 直到最近，测得的最大红移量是6.;3。
- Julie：Yeah.the problem is thisT-shirt.It’sdark blue .Pat：is it Liz’s？Julie:Actually .it‘smy T-shirt.I’m sorry.Pat: That’s OKIt‘not important. 朱莉:是啊.;这是T恤的问题
- The relationship between the pulse FWHM and fluence(flux) of FRED pulse light curves of GRBs was explored. 探讨了FRED脉冲型GRB光变曲线FWHM与光子流量以及光子峰值流量之间的关系.
- In fact, astronomers attribute long GRBs to collimated jets generated by rapidly spinning black holes. 事实上，天文学家把长GRB归因于快速旋转的黑洞所产生的平行喷流。
- The relationship between the pulse FWHM and fluence (flux) of FRED pulse light curves of GRBs was explored. 摘要探讨了FRED脉冲型GRB光变曲线FWHM与光子流量以及光子峰值流量之间的关系。
- Due to their huge luminosity, high redshift GRBs can be important as a probe of cosmology. 由于伽玛暴巨大的光度，高红移的伽玛暴对于宇宙学研究有重要意义。
- Until recently, experts were grappling with an even more fundamental question about GRBs: what the heck are they? 直到最近，专家们才确定抓住了GRB爆发的根本问题：它们到底是什么？
- The afterglow from some GRBs observed by the Italian/Dutch satellite BeppoSAX has strong confirmed the cosmological origin. 1997年以来，由于意大利和荷兰合作研制的BeppoSAX卫星的杰出贡献，人们观察到了一些伽玛射线暴的余辉，证实了它们的宇宙学起源。
- GrB positive cells in the liver mostly consisted of CD57 positive cells and a few CD3 positive cells. 在肝脏GrB阳性细胞中;大部分为CD57阳性细胞;少量为CD3阳性细胞.
- Intriguingly, the highest-energy gamma rays from this GRB arrived later than the low-energy gamma rays. 不过令人疑惑的是，爆发产生的低能伽马射线竟然早于超高能伽马射线到达地球。
- The discovery and consequent detailed observations of GRB afterglows strongly support the cosmological origin. 余辉的发现和随后的深入观测证实伽玛射线暴产生于宇宙学距离上。
- It has been found that that the polarization of GRB could be explained by pinch discharge model. 并利用箍缩模型解释了伽马暴的极化现象。
- Great progress on Gamma-ray burst (GRB) research has been made since the discovery of afterglows in 1997. g射线暴(简称g暴)的研究自1997年以来由于余辉的发现而有了很大的突破。
- S.A., a corporation listed on the New York Stock Exchange under the “GRB” symbol. 格柏科学集团公司是美国纽约股票交易所的上市公司，股票交易代码为 GRB。
- Long GRBs are therefore different than many types of supernovas, which occur more uniformly distributed in their host galaxies. 因此长期爆发的伽马射线与许多类型的超新星爆发不同，超新星爆发更多的是均一分布在它们的主星系内。
