Simultaneous multifrequency single-pulse properties of AXP XTE J1810–197 |
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| Authors: | M Serylak B W Stappers P Weltevrede M Kramer A Jessner A G Lyne C A Jordan K Lazaridis J A Zensus |
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| Institution: | Netherlands Institute for Research in Astronomy, Postbus 2, 7990 AA Dwingeloo, the Netherlands;Astronomical Institute 'Anton Pannekoek', University of Amsterdam, Kruislaan 403, 1098 SJ Amsterdam, the Netherlands;Jodrell Bank Observatory, University of Manchester, Macclesfield, Cheshire SK11 9DL;Australia Telescope National Facility, CSIRO, PO Box 76, Epping NSW 1710, Australia;Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, 53121 Bonn, Germany |
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| Abstract: | We have used the 76-m Lovell, 94-m equivalent Westerbork Synthesis Radio Telescope (WSRT) and 100-m Effelsberg radio telescopes to investigate the simultaneous single-pulse properties of the radio emitting magnetar Anomalous X-ray Pulsar (AXP) XTE J1810?197 at frequencies of 1.4, 4.8 and 8.35 GHz during 2006 May and July. We study the magnetar's pulse-energy distributions which are found to be very peculiar as they are changing on time-scales of days and cannot be fit by a single statistical model. The magnetar exhibits strong spiky single giant-pulse-like subpulses, but they do not fit the definition of the giant pulse or giant micropulse phenomena. Measurements of the longitude-resolved modulation index reveal a high degree of intensity fluctuations on day-to-day time-scales and dramatic changes across pulse phase. We find the frequency evolution of the modulation index values differs significantly from what is observed in normal radio pulsars. We find that no regular drifting subpulse phenomenon is present at any of the observed frequencies at any observing epoch. However, we find a quasi-periodicity of the subpulses present in the majority of the observing sessions. A correlation analysis indicates a relationship between components from different frequencies. We discuss the results of our analysis in light of the emission properties of normal radio pulsars and a recently proposed model which takes radio emission from magnetars into consideration. |
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| Keywords: | stars: neutron pulsars: general pulsars: individual: AXP J1810–197 |
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