Jump to content

PSR J1951+1123

From Wikipedia, the free encyclopedia

This is an old revision of this page, as edited by Loooke (talk | contribs) at 01:38, 3 April 2017 (forgot {{DEC). The present address (URL) is a permanent link to this revision, which may differ significantly from the current revision.

PSR J1951+1123
Observation data
Epoch J2000      Equinox J2000
Constellation Aquila
Right ascension 19h 51m 08.25s
Declination +11° 23′ 25.2"″
Characteristics
Spectral type Pulsar
Astrometry
Distance5216 ly
(1660 pc)
Details
Rotation5.09 s
Database references
SIMBADdata

PSR J1951+1123 is a pulsar. This pulsar is notable due to its exceptionally long period, one of the longest known, with a period of 5.09 seconds.[1]

References

  1. ^ Young, M. D.; Manchester, R. N.; Johnston, S. (1999). "A radio pulsar with an 8.5-second period that challenges emission models". Nature. 400 (6747): 848. Bibcode:1999Natur.400..848Y. doi:10.1038/23650.

External links