Abstract
An interferometric search for continuum radio emission from the Hulse- Taylor binary pulsar made with the NRAO interferometer at 2695 and 8085 MHz has resulted in the detection of a weak source well within the positional error box of the binary pulsar and a relatively strong source several arc minutes outside the error box.
Full Text 
Sign-in/Register to access full text options
Sign-in/Register to access full text options 
Published version (
Free)
Free) 
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
