Astronomy and Astrophysics – Astrophysics
Scientific paper
2002-04-26
Mon.Not.Roy.Astron.Soc. 333 (2002) L7
Astronomy and Astrophysics
Astrophysics
4 pages, 3 figures, accepted by MNRAS Letters
Scientific paper
10.1046/j.1365-8711.2002.05600.x
PSR J1806-2125 is a pulsar discovered in the Parkes multibeam pulsar survey with a rotational period of 0.4s and a characteristic age of 65kyr. Between MJDs 51462 and 51894 this pulsar underwent an increase in rotational frequency of $\Delta \nu/\nu \approx 16 \times 10^{-6}$. The magnitude of this glitch is approximately 2.5 times greater than any previously observed in any pulsar and 16 times greater than the mean glitch size. This letter gives the parameters of the glitch and compares its properties to previously observed events. The existence of such large and rare glitches offers new hope for attempts to observe thermal X-ray emission from the internal heat released following a glitch, and suggests that pulsars which previously have not been observed to glitch may do so on long timescales.
Camilo Fernando
D'Amico Nichi
Hobbs George
Joshi Bhal Chandra
Kaspi Victoria M.
No associations
LandOfFree
A Very Large Glitch in PSR J1806-2125 does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with A Very Large Glitch in PSR J1806-2125, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A Very Large Glitch in PSR J1806-2125 will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-397042