Spectral evolution and polarization of variable structures in the pulsar wind nebula of PSR B0540-69.3

Monthly Notices of the Royal Astronomical Society(2011)

引用 16|浏览11
暂无评分
摘要
We present high spatial resolution optical imaging and polarization observations of the PSR B0540−69.3 and its highly dynamical pulsar wind nebula (PWN) performed with Hubble Space Telescope, and compare them with X-ray data obtained with the Chandra X-ray Observatory. In particular, we have studied the bright region south-west of the pulsar where a bright ‘blob’ is seen in 1999. In a recent paper...
更多
查看译文
关键词
pulsars: individual: PSR B0540−69.3,supernovae: general,ISM: individual objects: SNR 0540−69.3,ISM: supernova remnants,Magellanic Clouds
AI 理解论文
溯源树
样例
生成溯源树,研究论文发展脉络
Chat Paper
正在生成论文摘要