Abstract
High-resolution observations of G292.0 + 1.8 made with the Fleurs synthesis telescope at 1415 MHz give no indication of a shell structure, but show a concentration towards the centre. The source therefore appears to belong to an unusual class of supernova remnants of which the Crab nebula is the best known. Comparisons are made with other supernova remnants of this type.
Full Text 
Sign-in/Register to access full text options
Sign-in/Register to access full text options 
Paper version not known
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a call
