| dc.contributor.author | Koen, Chris | |
| dc.date.accessioned | 2023-02-10T07:36:23Z | |
| dc.date.available | 2023-02-10T07:36:23Z | |
| dc.date.issued | 2007 | |
| dc.identifier.citation | Koen, 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.x | en_US |
| dc.identifier.issn | 1365-2966 | |
| dc.identifier.uri | https://doi.org/10.1111/j.1365-2966.2007.11684.x | |
| dc.identifier.uri | http://hdl.handle.net/10566/8404 | |
| dc.description.abstract | HE 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.language.iso | en | en_US |
| dc.publisher | Oxford University Press | en_US |
| dc.subject | Statistics studies | en_US |
| dc.subject | Subdwarf star | en_US |
| dc.subject | Binaries | en_US |
| dc.subject | South Africa | en_US |
| dc.subject | Astronomy | en_US |
| dc.title | HE 0230–4323: An unusual pulsating hot subdwarf star | en_US |
| dc.type | Article | en_US |
