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NLTE wind models of hot subdwarf stars

✍ Scribed by Jiří Krtička; Jiří Kubát


Publisher
Springer Netherlands
Year
2010
Tongue
English
Weight
459 KB
Volume
329
Category
Article
ISSN
0004-640X

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Observational asteroseismology of hot su
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## Abstract Hot subdwarf stars are particularly challenging for asteroseismology due to their rapid pulsation periods, intrinsic faintness and relative rarity both in the field and in clusters. These features have ensured that the preferred method of observation up to now has been white‐light photo