光变曲线的谷
现在一般都只看光变曲线的峰值，看峰值对应着什么过程。而光变的谷却没有人关心。
至少，如果光变曲线的谷不是零，就说明在那个时候源依然有辐射。
那可以从谷中挖些什么信息呢？
伽玛暴(Gamma-Ray Burst)笔记。记录有关伽玛暴的新文章，另外也包括看的老文章、自己的想法、以及跟天文相关的一些东西。 Feel free to leave me a message by comments or by email.
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2007
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- Sakamoto 2007 Swift BAT编目
- Kocevski 2007 Swift暴的能量
- Ramirez-Ruiz 2007 数值模拟正负电子对进入外部介质时的激波和磁场产生
- Huang 2007 伽玛暴的非相对论阶段
- Piro 2007 EDGE望远镜的设想
- Brown 2007 有几个银河系的源可能是伽玛暴的遗迹
- Eichler 2007 对暴本身阶段光变的FRED的解释
- Jóhannesson 2007 标准模型下伽玛暴余辉的光度函数
- Yost 2007 ROTSE-III暴本身阶段的光学观测
- Urata 2007 有一些暴的“正常”阶段也不能用标准余辉模型解释
- Chen 2007 通过伽玛暴余辉的谱定星系的Escape Fraction
- Li 2007 SN 1998bw 的射电光变
- Grrasberg 1971 超新星光变曲线理论
- Iwamoto 1994 SN 1994I光变曲线的理论计算
- Vianello 2007 GRB 061019 and GRB 070129的尘埃散射
- Nomoto 2007 伽玛暴与超新星的关联
- Nomoto 2007 贫金属坍缩超新星与伽玛暴的关联
- Sakamoto 2007 Swift暴快下降阶段的数据统计
- Bucciantini 2007 伽玛暴的磁星模型
- Vetere 2007 BeppoSAX 1996-2002的所有数据
- Uzdensky 2007 磁场主导的喷流作为超新星和伽玛暴的爆发机制
- Zhang 2007 伽玛暴光变的时间特性
- Cuesta 2007 伽玛暴在Gurzadyan-Xue的宇宙学模型中的应用
- Murase 2007 早期余辉阶段的高能中微子
- De Rujula 2007 Swift观测继续验证canonball模型
- 用050904的模型拟合XRFs的光变曲线
- 中子星磁场的消失作为伽玛暴的能源
- 光变曲线的谷
- 黑体辐射是效率最高的吗
- 通过超新星的光变推测爆发时间
- 黄山会议印象－学术版
- Genet 2007 对GRB 050820a的拟合
- Daigne 2007 低光度GRB980425的两种可能解释
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