Optical Candidate for Pulsar PSR 0833-45

Details Optical Candidate for Pulsar PSR 0833-45 Optical Candidate for Pulsar PSR 0833-45

Apr 1969

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1969natur.222..359c&link_type=abstract

Nature, Volume 222, Issue 5191, pp. 359 (1969).

Physics

5

Scientific paper

Two of the most singular characteristics of the pulsar NP 0532 are its
short period (33 ms) and its association with a supernova remnant. This
suggests that the next most promising candidate for detection of optical
radiation from a pulsar is PSR 0833-45 (ref. 1), associated with the
supernova remnant in Vela, which has a period of 89 ms.

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