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Observational aspects of chromospheres and coronae in hot stars

✍ Scribed by R. Stalio


Publisher
Elsevier Science
Year
1983
Tongue
English
Weight
859 KB
Volume
2
Category
Article
ISSN
0273-1177

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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