Multiwavelength view of J1740+1000. Purple indicates the ultrahigh-energy gamma-ray emission measured with LHAASO. (IMAGE)

Chinese Academy of Sciences Headquarters

Multiwavelength view of J1740+1000. Purple indicates the ultrahigh-energy gamma-ray emission measured with LHAASO.

Caption

Red shows the partial X-ray tail of the pulsar wind nebula measured with the XMM-Newton satellite (left), and blue shows the complete X-ray tail of the pulsar wind nebula observed with Einstein Probe (right). Although XMM-Newton's observing time was more than six times that of Einstein Probe, it detected only a small fraction of the tail.

Credit

Credit: Y.-H. Chi et al.

Usage Restrictions

News organizations may use or redistribute this image, with proper attribution, as part of news coverage of this paper only.

License

Original content

Disclaimer: AAAS and EurekAlert! are not responsible for the accuracy of news releases posted to EurekAlert! by contributing institutions or for the use of any information through the EurekAlert system.