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Interferometric search for the Hulse--Taylor binary pulsar

Journal Article · · Astrophys. J., Lett., v. 199, no. 3, pp. L165-L166
DOI:https://doi.org/10.1086/181874· OSTI ID:4170963
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.
Research Organization:
National Radio Astronomy Observatory, Charlottesville, Virginia
Sponsoring Organization:
USDOE
NSA Number:
NSA-33-001533
OSTI ID:
4170963
Journal Information:
Astrophys. J., Lett., v. 199, no. 3, pp. L165-L166, Journal Name: Astrophys. J., Lett., v. 199, no. 3, pp. L165-L166; ISSN AJLEA
Country of Publication:
United States
Language:
English

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