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标题：Just how hot are the ω Centauri extreme horizontal branch pulsators?
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作者：M. Latour ; M. Latour ; S. K. Randall 等
期刊名称：Astronomy & Astrophysics
印刷版ISSN：0004-6361
电子版ISSN：1432-0746
出版年度：2017
卷号：600
页码：1-8
DOI：10.1051/0004-6361/201630132
语种：English
出版社：EDP Sciences
摘要：Context. Past studies based on optical spectroscopy suggest that the five ω Cen pulsators form a rather homogeneous group of hydrogen-rich subdwarf O stars with effective temperatures of around 50 000 K. This places the stars below the red edge of the theoretical instability strip in the log g−Teff diagram, where no pulsation modes are predicted to be excited. Aims. Our goal is to determine whether this temperature discrepancy is real, or whether the stars’ effective temperatures were simply underestimated. Methods. We present a spectral analysis of two rapidly pulsating extreme horizontal branch (EHB) stars found in ω Cen. We obtained Hubble Space Telescope/COS UV spectra of two ω Cen pulsators, V1 and V5, and used the ionisation equilibrium of UV metallic lines to better constrain their effective temperatures. As a by-product we also obtained FUV lightcurves of the two pulsators. Results. Using the relative strength of the N iv and N v lines as a temperature indicator yields Teff values close to 60 000 K, significantly hotter than the temperatures previously derived. From the FUV light curves we were able to confirm the main pulsation periods known from optical data. Conclusions. With the UV spectra indicating higher effective temperatures than previously assumed, the sdO stars would now be found within the predicted instability strip. Such higher temperatures also provide consistent spectroscopic masses for both the cool and hot EHB stars of our previously studied sample.
关键词：stars: atmospheres;stars: fundamental parameters;subdwarfs;globular clusters: individual: omega Centauri;stars: variables: general;stars: horizontal-branch