An unusual glitch signature in the pulsar PSR B1822-09

Details An unusual glitch signature in the pulsar PSR B1822-09 An unusual glitch signature in the pulsar PSR B1822-09

Sep 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998a%26a...337..723s&link_type=abstract

Astronomy and Astrophysics, v.337, p.723-728 (1998)

Astronomy and Astrophysics

Astrophysics

19

Pulsars: General, Pulsars: Individual: Psr B1822-09, Stars: Rotation

Scientific paper

Two glitches have been detected in the pulsar PSR B1822-09. The first glitch occurred around MJD 49615 and was characterized by a fractional increase in rotational frequency of 2{x}10(-10) . The second glitch occurred 325 days after the first one and caused a fractional change in frequency of 5{x}10(-9) . Of interest was the post-glitch behaviour. The rotational frequency immediately after the second glitch began slowly, gradually increasing which lasted { ~ }620 days. As a result of the slow increase a fractional change in rotation frequency for this period of time made up 7{x}10(-9) . This event was accompanied by a decrease in the frequency derivative, which having reached minimum magnitude { ~ }0.4{%} less than the original value, returned to its initial value.

Affiliated with

Also associated with

No associations

Rating

An unusual glitch signature in the pulsar PSR B1822-09 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 An unusual glitch signature in the pulsar PSR B1822-09, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and An unusual glitch signature in the pulsar PSR B1822-09 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-810196