Astronomy and Astrophysics – Astrophysics
Scientific paper
Feb 1975
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975apj...196...83m&link_type=abstract
Astrophysical Journal, vol. 196, Feb. 15, 1975, pt. 1, p. 83-102.
Astronomy and Astrophysics
Astrophysics
124
Extragalactic Radio Sources, Polarization Characteristics, Pulsars, Pulsed Radiation, Radio Emission, Angular Distribution, Circular Polarization, Longitude, Orthogonality, Polarized Radiation, Self Absorption, Very High Frequencies
Scientific paper
Observations of complete polarization characteristics of individual pulses in the frequency range from 110 to 450 MHz are reported for twelve pulsars along with the linear polarization characteristics at 1400 MHz for four pulsars. Subpulses were found to be mostly linearly polarized, with the variation of position angle within a subpulse usually less than 30 deg. In many pulsars at low frequencies the position angle of successive subpulses is stable for most of the profile. For certain components, however, subpulses are observed with position angle orthogonal to the most common angle. An interpretation based on self-absorption in the emission region is given.
Huguenin Richard G.
Manchester Richard N.
Taylor Joseph H. Jr.
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