Radio observations of X-ray pulsators

Details Radio observations of X-ray pulsators Radio observations of X-ray pulsators

Jan 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983ap%26ss..89..169c&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 89, no. 1, Jan. 1983, p. 169-172.

Astronomy and Astrophysics

Astronomy

2

Pulsars, Radio Astronomy, Stellar Oscillations, X Ray Sources, Binary Stars, Emission Spectra, Magnetic Stars, Neutron Stars, Stellar Spectrophotometry, White Dwarf Stars

Scientific paper

A detailed search has been performed at 10.7 Ghz for any pulsed radio emission from four X-ray pulsators (A0535 + 26, X Persei, AE Aquarii and H2252-035). The results obtained indicate no radio emission-pulsed or otherwise is present at a level of at least 50 mJy (two standard deviations upper limit). This value is considerably more sensitive than the previous studies carried out on these sources and presents problems in the understanding of compact, magnetized stellar objects.

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