Detection of radio emission from the AXP 4U 0142+61 |
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Authors: | V M Malofeev D A Teplykh O I Malov |
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Institution: | (1) P.N.Lebedev Physical Institute, Russian Academy of Sciences, Pushchino, Moscow region, PRAO FIAN, 142290, Russia |
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Abstract: | The detection of pulsed radio emission from the X-ray pulsar AXP 4U 0142+61 with a period of P = 8.68832935(6) s and a period derivative of $
\dot P
$
\dot P
= 18.713(4) × 10−13 s/s is reported. The observations were carried out on two high-sensitivity radio telescopes of the Pushchino Radio Astronomy
Observatory: the Large Phased Array at 111MHz and the DKR-1000 at 40MHz.Mean pulse profiles are presented; the measured flux
density is S
111 = 30 ± 20 mJy. The estimated distance derived from the dispersion measure, 27 pc/cm3, is 1.4 kpc, and the integrated radio luminosity is L
R
= 1.5 × 1027 erg/cm. Comparison with X-ray data shows an appreciable difference in the pulse duration (the radio pulse is about a factor
of 20 more narrow) and strong variations in the flux density. |
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Keywords: | |
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