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Infrared observational study of MS and CS stars

✍ Scribed by Pei-sheng Chen; Heng Gao; Chu-xian Bao; Yan-kang Chen

Publisher
Elsevier Science
Year
1991
Tongue
English
Weight
447 KB
Volume
15
Category
Article
ISSN
0275-1062

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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