HE 0230–4323: An unusual pulsating hot subdwarf star

dc.contributor.authorKoen, Chris
dc.date.accessioned2023-02-10T07:36:23Z
dc.date.available2023-02-10T07:36:23Z
dc.date.issued2007
dc.description.abstractHE 0230−4323 is a known binary, consisting of a subdwarf star and a companion which is not observable in the optical. Photometric measurements reported in this paper have shown it to be both a reflection-effect and a pulsating variable. The dominant pulsation frequencies changed over the course of several nights of observing, from ∼32–39 d−1 to ∼8–16 d−1. Observations were obtained through B and V filters, and the variations in the two wavebands appear to be approximately 180◦ out of phase.en_US
dc.identifier.citationKoen, C. (2007). HE 0230–4323: An unusual pulsating hot subdwarf star. Monthly Notices of the Royal Astronomical Society, 377(3), 1275–1280. https://doi.org/10.1111/j.1365-2966.2007.11684.xen_US
dc.identifier.issn1365-2966
dc.identifier.urihttps://doi.org/10.1111/j.1365-2966.2007.11684.x
dc.identifier.urihttp://hdl.handle.net/10566/8404
dc.language.isoenen_US
dc.publisherOxford University Pressen_US
dc.subjectStatistics studiesen_US
dc.subjectSubdwarf staren_US
dc.subjectBinariesen_US
dc.subjectSouth Africaen_US
dc.subjectAstronomyen_US
dc.titleHE 0230–4323: An unusual pulsating hot subdwarf staren_US
dc.typeArticleen_US

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