Astronomy and Astrophysics – Astronomy
Scientific paper
Dec 1996
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996astl...22..811s&link_type=abstract
Astronomy Letters, Vol. 22, No. 6, p. 811-814; Pis'ma v Astronomicheskii Zhurnal, Vol. 22, p. 905
Astronomy and Astrophysics
Astronomy
1
Pulsars: Radio Radiation, Pulsars: Pulse Profiles
Scientific paper
Observations of the pulsar PSR 0943+10 at 40 MHz (Pushchino, Russia) and 430 MHz (Arecibo, USA) have revealed a process that is a precursor to bursts of either of the two modes of radio emission of the pulsar pulses. In PSR 0943+10, a new mode is preceded by a gradual decrease in the intensity of the pulses, which gives way to a rapid decay one minute before a sharp switch from one mode to the other and which lasts for some time after this event. Variations in the intensity of the pulsar radio emission during the mode switching appear to be caused by the relaxation of a hot spot on the surface of the neutron star.
Izvekova Vera A.
Sulejmanova S. A.
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