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PSR J0537−6910

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(Redirected fromPSR J0537-6910)
Star in the constellation Dorado
This article includes a list ofgeneral references, butit lacks sufficient correspondinginline citations. Please help toimprove this article byintroducing more precise citations.(June 2022) (Learn how and when to remove this message)
PSR J0537-69
Observation data
Epoch J2000      Equinox J2000
ConstellationDorado
Right ascension05h 37m 47.6s
Declination−69° 10′ 20″
Characteristics
Spectral typePulsar
Variable typeNone
Astrometry
Distance170,000ly
Details
Rotation0.016129s
Age4,000 years
Other designations
PSR J0537-69,CXOU J053747.3-691020,XMMU J053747.4-691020,CXOU J053747.4-691019,PSR J0537-6910, [CWG2006] 4.
Database references
SIMBADdata

PSR J0537-6910 is apulsar that is 4,000 years old (not including the light travel time toEarth). It is located about 170,000light-years away, in the southernconstellation ofDorado, and is located in theLarge Magellanic Cloud. It rotates at 62hertz.

A team atLANL advanced that it is possible to predictstarquakes in J0537-6910,[1] meaning that it may be possible to devise a way to forecastglitches at least in some exceptional pulsars.[2] The same team observed magnetic pole drift on this pulsar with observational data fromRossi X-ray Timing Explorer.

References

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  1. ^Middleditch, John; Marshall, Francis E.; Wang, Q. Daniel; Gotthelf, Eric V.; Zhang, William (December 2006). "Predicting the Starquakes in PSR J0537-6910".The Astrophysical Journal.652 (2):1531–1546.arXiv:astro-ph/0605007.Bibcode:2006ApJ...652.1531M.doi:10.1086/508736.ISSN 0004-637X.
  2. ^Antonelli, Marco; Montoli, Alessandro; Pizzochero, Pierre (November 2022), "Insights into the Physics of Neutron Star Interiors from Pulsar Glitches",Astrophysics in the XXI Century with Compact Stars, pp. 219–281,arXiv:2301.12769,doi:10.1142/9789811220944_0007,ISBN 978-981-12-2093-7,S2CID 256390487

External links

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See also

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