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Observational study of interacting binary stars

✍ Scribed by Tae Seog Yoon; Jeong Ae Lee; Jae Gyu Byeon; Kang Min Kim; Jin Hyung Kim; Kye Hwa Yoo; Soo Hyun Kim

Publisher
Elsevier Science
Year
2004
Tongue
English
Weight
209 KB
Volume
48
Category
Article
ISSN
1387-6473

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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