High-sensitivity observations of 28 pulsars

Details High-sensitivity observations of 28 pulsars High-sensitivity observations of 28 pulsars

Sep 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986aj.....92..621w&link_type=abstract

Astronomical Journal (ISSN 0004-6256), vol. 92, Sept. 1986, p. 621-626.

Mathematics

Logic

26

Pulsars, Stellar Spectrophotometry, Emission Spectra, Spectral Sensitivity, Stellar Cores, Stellar Structure

Scientific paper

Average 430 MHz pulse profiles and, where possible, modulation indices and pulse-nulling fractions are computed for 28 pulsars. Morphological classifications are determined for most of the pulsars. The authors find that core emission components tend to have lower modulation indices than conal components and that pulsars having only a core component never exhibit pulse nulling. PSR 1612+07 is shown to undergo mode changes.

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