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Stokes tomography of radio pulsar magnetospheres. I. Linear polarization
Solar and Stellar Astrophysics (astro-ph.SR)
2011/1/4
Polarimetric studies of pulsar radio emission traditionally concentrate on how the Stokes vector (I, Q, U, V) varies with pulse longitude, with special emphasis on the position angle (PA) swing of the...
The optical counterpart of sax j1808.4{3658 in quiescence：evidence of an active radio pulsar?
sax j1808.4{3658 radio pulsar
2009/6/17
The optical counterpart of sax j1808.4{3658 in quiescence：evidence of an active radio pulsar?