Main Pulse / Interpulse Correlation and Mode Changing in PSR:1055-52

Details Main Pulse / Interpulse Correlation and Mode Changing in PSR:1055-52 Main Pulse / Interpulse Correlation and Mode Changing in PSR:1055-52

Sep 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990mnras.246..341b&link_type=abstract

Monthly Notices of the Royal Astronomical Society, Vol. 246, NO.2/SEP15, P. 341, 1990

Astronomy and Astrophysics

Astronomy

17

Scientific paper

We have studied the individual pulses from PSR 1055-52, a pulsar which has a strong interpulse. Their properties, and those of the average pulse profile, are consistent with an emission geometry in which the magnetic and rotation axes are nearly orthogonal. That is, we are observing both magnetic poles of this pulsar. A correlation between emission from the two magnetic poles was found wherein a strong interpulse is followed by a strong main pulse. We discuss possible agencies for this one-way communication between the magnetic poles. Also, the main pulse appears to undergo mode changes that are primarily characterized by a change in peak flux density of component I.

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