Sie befinden Sich nicht im Netzwerk der Universität Paderborn. Der Zugriff auf elektronische Ressourcen ist gegebenenfalls nur via VPN oder Shibboleth (DFN-AAI) möglich. mehr Informationen...
Astrophysics and space science, 2019-10, Vol.364 (10), p.1-6, Article 173
Ort / Verlag
Dordrecht: Springer Netherlands
Erscheinungsjahr
2019
Quelle
Alma/SFX Local Collection
Beschreibungen/Notizen
We present a timing analysis of PSR J1602–5100 using approximately seven years of observations from the Parkes 64-m radio telescope. A slow glitch that occurred between 2008 September 24 and 2010 May 14 (MJDs 54733 and 55330) is identified. During this time, the pulsar showed a slow exponential growth in the spin frequency
ν
, and the spin-down rate
|
ν
˙
|
suddenly decreased to a peak value, followed by a linear return to its initial value. Our measurements of the maximum
Δ
ν
and
Δ
ν
˙
are
176
nHz
and
3.58
×
10
−
15
s
−
2
, corresponding to fractional sizes of
152
×
10
−
9
(
Δ
ν
/
ν
)
and
−
38.6
×
10
−
3
(
Δ
ν
˙
/
ν
˙
)
, respectively. This is the largest slow glitch observed so far. Moreover, more complex changes in the shape of the pulse profile are considered to be associated with this unusual glitch activity.