Relationships between the Three Types of Pulse Lags in Long-Iag GRBs
We calculate the three types of pulse lags in longlag GRBs with the pulse peaking time (tpeak), the pulse centroid time (tcen), and the cross-correlation function (CCF). We find that the lag calculated by CCF is strongly correlated with that derived from tpek, while the lag derived from tcen is less correlated with that derived from tpeak and CCF. In addition, the centroid lag is systematically larger than both the peak lag and the CCF lag. It is possible that the different types of lag measurements could be used as a tool for probing aspects of pulse evolution.
gamma-rays bursts
Fu-Wen zhang
Department of Maths and Physics, Guilin University of Technology, Guilin, Guangxi 541oo4, China National Astronomical Observatories/Yunnan Observatorli, Chinese Academy of Sciences, Kunming, Yunnan 650011, China
国际会议
The 10th Asian-Pacific Regional International Astronomical Union Meeting(第十届亚洲及太平洋地区天文学大会 APRIM)
昆明
英文
278-279
2008-08-03（万方平台首次上网日期，不代表论文的发表时间）