Separation of the polarization modes in PSR 0823 + 26

Details Separation of the polarization modes in PSR 0823 + 26 Separation of the polarization modes in PSR 0823 + 26

Feb 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991a%26a...242..119g&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 242, no. 1, Feb. 1991, p. 119-124. Research supported by Polish Academy of Sci

Astronomy and Astrophysics

Astrophysics

18

Polarized Electromagnetic Radiation, Pulsars, Stellar Radiation, Error Analysis, Polarization Characteristics

Scientific paper

A 1404-MHz polarization observation of PSR 0823 + 26 is studied in order
to separate the two different polarization modes. The modes are
significantly nonorthogonal in the central parts of the profile. It is
argued that the nonorthogonal separation between the modes is associated
with an inconsistency of the weaker mode with the rotating vector model.

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