Astronomers are baffled by what may be the tail of a spinning neutron star or pulsar named PSR JO357+3205, whose brightest point is well away from the star. Further observations by the Chandra X-ray Observatory and other telescopes are planned. Credit: NASA/CXC/A. Hobart
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This recording of the pulsar CP1133 was received on May 9th 1968 at Aricebo Radio Telescope in Puerto Rico. The receiver was tuned to 111.5 MHz with a resolution bandwidth of 300 kHz and a video bandwidth of 3 kHz. This pulsar has a period of 1.1878 seconds. Recording kindly provided by Bob K5DZE.
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