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A&A 500, 861-865 (2009)
DOI: 10.1051/0004-6361/200911648
The emission polarization of RX J1856.5-3754
N. ChkheidzeTbilisi State University, Chavchavadze Avenue 3, 0128, Tbilisi, Georgia
e-mail: n.chkheidze@gmail.com
Received 12 January 2009 / Accepted 18 March 2009
Abstract
The polarization properties of RX J1856.5-3754 are
investigated, based on the plasma emission model presented in
previous works. It is shown that if the emission of this source is
generated by the synchrotron mechanism, then the X-ray and the
optical emission should be linearly polarized and the corresponding
degrees of linear polarization are calculated. The change of the
position angle through the observable period is investigated.
According to the model, the position angle should undergo a
full-circle rotation more than once within this period. This unusual
behaviour of the position angle is a prediction of the model and its
detection would be a strong argument in favour of it. The
measurement of the polarization patterns of this source appears to
be the most reliable way to make clear its real emission nature.
Key words: stars: pulsars: individual: RX J1856.5-3754 -- radiation mechanisms: non-thermal -- polarization
© ESO 2009
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