``Inverse mapping'' of non thermal optical emission from isolated neutron stars

Details ``Inverse mapping'' of non thermal optical emission from isolated neutron stars ``Inverse mapping'' of non thermal optical emission from isolated neutron stars

Oct 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001aipc..586..565o&link_type=abstract

RELATIVISTIC ASTROPHYSICS: 20th Texas Symposium. AIP Conference Proceedings, Volume 586, pp. 565-568 (2001).

Astronomy and Astrophysics

Astrophysics

Neutron Stars, Stellar Atmospheres, Radiative Transfer, Opacity And Line Formation, Mathematical Procedures And Computer Techniques, Pulsars, Magnetic And Electric Fields, Polarization Of Starlight, Radiation Mechanisms, Polarization, Visible

Scientific paper

The region(s) within the magnetosphere where the IR-->UV emissions arise is essentially unknown. This work is an attempt to place constraints on possible emission regions using a computationally intensive, ``inverse mapping'' approach. This approach can yield a localisation of emission regions within the magnetosphere and also gives an estimate of pulsar inclination angles. Initial results for PSR B0531+21 (the Crab) are presented. .

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