Detection of giant component from pulsar PSR J0653+8051 V.M. Malofeev, D.A. Teplykh, O.I. Malov and S.V. Logvinenko Pushchino Radio Astronomy Observatory.

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Presentation transcript:

Detection of giant component from pulsar PSR J V.M. Malofeev, D.A. Teplykh, O.I. Malov and S.V. Logvinenko Pushchino Radio Astronomy Observatory ASC LPI RAS

Observations of B in 1996 Malofeev et al., 1998

Observations LPA : LPA : ± 1.5 МHz, 3.3 m / cos , A ef  m 2 Digital receiver: 512  5 kHz,  t  2.45; 5.12 ms Apr.2012 – Apr observation sessions 1 observation session = 994 periods B (J ) p = 1,214 s p' = 3, s/s T = years B = G DM = 32,5 pc/cm 3

Examples of integrated profiles S/n < 326.5% < S/n < 562% S/n > 512% Intensity in arbitrary units Pulse longitude (samples) S/n > 100,4%

The fluctuations of the component intensity

Outburst ( ) Sum of 408 double periods Integrated pulse profile Sum of 816 pulses Intensity Frequency Pulse longitude (samples)

Outburst ( ) Sum of 378 pulses: S/n(C2) < 5 Sum of 31 pulses: S/n(C1, C3) > 2,5, S/n(C2) < 5 Sum of 32 pulses: S/n > 5 C1 C2 C3 Intensity in arbitrary units Intensity Pulse longitude (samples) = 80 deg 158 pulses (C2 – 134) S/n ≥ pulses (C2 – 56) S/n ≥ 5 16 pulses (C2 – 16) S/n ≥ 10

Intensity variations of pulses during “outburst” sessions Pulse number Pulse longitude in sample (1 sample = 5,12 ms) Double period Pulse number Pulse longitude in sample (1 sample = 5,12 ms) Double period

Intensity variations of pulses during session of Pulse number Pulse longitude in sample (1 sample = 5,12 ms) Double period C1 C2 C3 Sum of 439 double pulses Sum of 30 double pulses Sum of 495 double pulses

The examples of the individual pulses ( ) C1 C2 C3 Intensity in arbitrary units Pulse longitude (samples) = 80 deg

The dispersion slope in time-frequency plane frequency Time (2 periods) 16 pulses

Nature of events

Summary  We confirmed the presence of the bursts in second component of three-components profile (Malofeev et al., 1998)  We detected that intensity of this component can be a factor 170 higher than its mean value. The duration of the bursts is about 300 periods (~6 min) and such event is extremely rare ~ 0.01% of observing time  We find the long-time (a few months) variation of intensity of all components, then this value changed in two times with the average intensity of pulse emission.