|This article relies largely or entirely upon a single source. (June 2013)|
Epoch J2000 Equinox J2000
|Right ascension||21h 44m 12.10s|
|Declination||-39° 33' 55.2"'|
|U−B color index||?|
|B−V color index||?|
|Distance||587.088 Ly (180 parsecs)|
PSR J2144-3933 is a pulsar about 180 parsecs (5.5 Em) from Earth. It was previously thought to have a period of 2.84 seconds but is now known to have a period of 8.51 s, which is among the longest known radio pulsar.
J2144-3933 is notable for other reasons: its mean pulse profile is very narrow in comparison to the pulse period with a half-intensity width of less than one degree of longitude. It also has the lowest spindown luminosity of any pulsar at about 3×1021 watts.
- Moreover, under the usual model assumptions, based on the neutron-star equations of state, this slowly rotating pulsar should not be emitting a radio beam. Therefore either the model assumptions are wrong, or current theories of radio emission must be revised
- ""Undead" Star Torpedoes Current Theories". Sciencedaily.com. 26 August 1999. Retrieved June 2013. Check date values in:
- Kohler, Susanna (25 March 2011). "A Pulsar Alone: The first deep X-ray and optical observations of the closest isolated radio pulsar". Astrobites.org. Retrieved June 2013. Check date values in:
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