2016MNRAS.455..150U

Query : 2016MNRAS.455..150U

2016MNRAS.455..150U - Mon. Not. R. Astron. Soc., 455, 150-157 (2016/January-1)

Detection of the fine structure of the pulsar J0953+0755 radio emission in the decametre wave range.

ULYANOV O.M., SKORYK A.O., SHEVTSOVA A.I., PLAKHOV M.S. and ULYANOVA O.O.

Abstract (from CDS):

In this paper the anomalous intense pulse of PSR J0953+0755 was studied in the decametre wavelength range. For this pulse, two scales of fine structure were discovered. The long-scale structure consists of four components, where the visible dispersion measures of even and odd components are different. The obtained time-scale of the short fine structure is 1 ms. The difference in visible dispersion measure can be caused by propagation of two normal modes of the pulsar radiation and irregularities of electron concentration in the space near the neutron star-like upper layers of magnetosphere and pulsar wind.

Abstract Copyright: © 2015 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society (2015)

Journal keyword(s): magnetic fields - plasmas - polarization - pulsars: individual: J0953+0755

Simbad objects: 2

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Number of rows : 2
N Identifier Otype ICRS (J2000)
RA 		ICRS (J2000)
DEC 		Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026 		#notes
1 PSR B0809+74 Psr 08 14 59.500 +74 29 05.70           ~ 425 0
2 PSR B0950+08 Psr 09 53 09.31210 +07 55 36.9000           ~ 806 2

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