Rotating RAdio Transients: multiwavelength observations

摘要：

Rotating RAdio Transients are a new class of neutron stars discovered through the emission of radio bursts. Eleven sources are known up to now, but population studies predict these objects to be more numerous than the normal radio pulsar population. Multiwavelength observations of these peculiar objects are in progress to disentangle their spectral energy distribution, and then study in detail their nature. In this review Ⅰ will report on the current state of the art on these objects.

关键词： Pulsar Neutron Star X-ray IR Radio

作者: Nanda Rea Maura McLaughlin

作者单位: SRON Netherlands Institute for Space Research, Sorbonnelaan, 2, 3584 CA, Utrecht, NL University of A Department of Physics, West Virginia University, Morgantown, WV 26501 National Radio Astronomy Obser

会议类型: 国际会议

会议名称: 紧凑型物体的天体物理学国际会议(International Conference on Astrophysics of Compact Objects)

会议地点: 安徽黄山

会议语种:英文

页码: 151-158

在线出版日期: 2007-07-01（万方平台首次上网日期，不代表论文的发表时间）