2014MNRAS.444.2494O


Query : 2014MNRAS.444.2494O

2014MNRAS.444.2494O - Mon. Not. R. Astron. Soc., 444, 2494-2497 (2014/November-1)

Radio emission of magnetars driven by the quasi-linear diffusion.

OSMANOV Z.

Abstract (from CDS):

In this paper, we study the possibility of generation of electromagnetic waves in the magnetospheres of radio magnetars by means of the quasi-linear diffusion (QLD). Considering the magnetosphere composed of the so-called beam and the plasma components, respectively, we argue that the frozen-in condition will inevitably lead to the generation of the unstable cyclotron modes. These modes, via the QLD, will in turn influence the particle distribution function, leading to certain values of the pitch angles, thus to an efficient synchrotron mechanism, producing radio photons. We show that for three known radio magnetars, the QLD might be a realistic mechanism for producing photons in the radio band.

Abstract Copyright: © 2014 The Author Published by Oxford University Press on behalf of the Royal Astronomical Society (2014)

Journal keyword(s): plasmas - radiation mechanisms: non-thermal

Simbad objects: 6

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Number of rows : 6
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2024
#notes
1 PSR J0146+6145 Psr 01 46 22.21 +61 45 03.8   28.100 25.620     ~ 570 0
2 PSR J1550-5418 Psr 15 50 54.18 -54 18 23.9           ~ 409 1
3 PSR J1622-4950 Psr 16 22 44.80 -49 50 54.4           ~ 146 0
4 PSR J1745-2900 Psr 17 45 40.1640 -29 00 29.818           ~ 315 0
5 AX J1809.8-1943 Psr 18 09 51.07 -19 43 51.8           ~ 463 0
6 2E 4673 HXB 23 01 08.14 +58 52 44.5           ~ 633 1

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