𝔖 Bobbio Scriptorium
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IUE observations of hot stars

✍ Scribed by Peter S. Conti

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

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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