Possible model for a rapidly pulsating radio source


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ABSTRACT The pulsating radio signals may come from active regions on rapidly rotating white dwarf stars. This accounts for some aspects of the periodicity of the signals which are difficult


to explain if the sources are pulsating stars. Access through your institution Buy or subscribe This is a preview of subscription content, access via your institution ACCESS OPTIONS Access


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subscriptions * Read our FAQs * Contact customer support SIMILAR CONTENT BEING VIEWED BY OTHERS A RADIO TRANSIENT WITH UNUSUALLY SLOW PERIODIC EMISSION Article 26 January 2022 A LONG-PERIOD


RADIO TRANSIENT ACTIVE FOR THREE DECADES Article 19 July 2023 SPORADIC RADIO PULSES FROM A WHITE DWARF BINARY AT THE ORBITAL PERIOD Article Open access 12 March 2025 REFERENCES * Hewish, A.,


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Princeton, New Jersey JEREMIAH OSTRIKER Authors * JEREMIAH OSTRIKER View author publications You can also search for this author inPubMed Google Scholar RIGHTS AND PERMISSIONS Reprints and


permissions ABOUT THIS ARTICLE CITE THIS ARTICLE OSTRIKER, J. Possible Model for a Rapidly Pulsating Radio Source. _Nature_ 217, 1227–1228 (1968). https://doi.org/10.1038/2171227a0 Download


citation * Received: 18 March 1968 * Issue Date: 30 March 1968 * DOI: https://doi.org/10.1038/2171227a0 SHARE THIS ARTICLE Anyone you share the following link with will be able to read this


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