Decametre wavelength observations of PSR 0834+06 and PSR 1919+21

Details Decametre wavelength observations of PSR 0834+06 and PSR 1919+21 Decametre wavelength observations of PSR 0834+06 and PSR 1919+21

Jul 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987mnras.227..197h&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 227, July 1, 1987, p. 197-204.

Astronomy and Astrophysics

Astronomy

1

Decametric Waves, Pulsars, Radio Spectra, Stellar Spectrophotometry, Emission Spectra, Low Frequencies, Radio Telescopes

Scientific paper

The University of Tasmania decametric array radio telescope has been used to observe two well-known pulsars (PSR 0834+06 and PSR 1919+21) in an attempt to confirm the decametric interpulse emission reported by Soviet investigators. Evidence for such emission was found in a 39-MHz profile of PSR 0834+06, but 47 MHz observations of PSR 1919+21 do not indicate significant emission outside the main pulse window. Detailed low-frequency spectra for the two sources are also given.

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