On the polarization-modal construction of triplicity in the profile of pulsar 1604-00

Details On the polarization-modal construction of triplicity in the profile of pulsar 1604-00 On the polarization-modal construction of triplicity in the profile of pulsar 1604-00

Feb 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988apj...325..314r&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 325, Feb. 1, 1988, p. 314-319. Research supported by the Research Corp., Un

Astronomy and Astrophysics

Astrophysics

27

Polarization (Waves), Pulsars, Stellar Radiation

Scientific paper

Pulsar 1604-00 exhibits a narrow triple profile which at 430 MHz is barely resolved into three components. In order to determine where this profile was merely a statistical fluke or whether it has more fundamental causes in the star's sequences of individual pulses, polarization mode separation of the individual pulse train was undertaken. An intriguing result was obtained: the primary- and the secondary-mode average profiles exhibit conal-double- and core-single-like forms, respectively. The significance of this finding is discussed.

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