C.D.S. - SIMBAD4 rel 1.7 - 2020.12.03CET18:41:57

2011A&A...527A...2C - Astronomy and Astrophysics, volume 527A, 2-2 (2011/3-1)

The plasma emission model of RBS 1774.


Abstract (from CDS):

In the present paper we construct a self-consistent theory, interpreting the observational properties of RBS1774. It is well known that the distribution function of relativistic particles is one-dimensional at the pulsar surface. However, cyclotron instability causes an appearance of transverse momenta of relativistic electrons, which as a result, start to radiate in the synchrotron regime. We study the process of the quasi-linear diffusion developed by means of the cyclotron instability on the basis of the Vlasov's kinetic equation. This mechanism provides generation of measured optical and X-ray emission on the light cylinder lengthscales. A different approach of the synchrotron theory is considered, giving the spectral energy distribution that is in a good agreement with the XMM-Newton observational data. We also provide the possible explanation of the spectral feature at 0.7 keV, in the framework of the model.

Abstract Copyright:

Journal keyword(s): X-rays - stars: pulsars: individual: RBS1774 - radiation mechanisms: non-thermal

Simbad objects: 2

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Number of rows : 2

N Identifier Otype ICRS (J2000)
ICRS (J2000)
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2021
1 RX J1856.6-3754 N* 18 56 35.11 -37 54 30.5     25.7     ~ 391 0
2 RX J2143.0+0654 N*? 21 43 03.8 +06 54 20           ~ 73 0

    Equat.    Gal    SGal    Ecl

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