Abstract
The stability of the pulsation periods of the sdB pulsator HS 2201+2610 is analyzed after 15 months of photometric monitoring. Although the time basis is not long enough to obtain a measurement of P, an upper limit of about 4×10-12 (in absolute value) is derived for the variation of the main pulsation period in time.
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© 2003 Springer Science+Business Media Dordrecht
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Silvotti, R., Kalytis, R. (2003). Pulsation Period Stability in the SDBV Star HS 2201+2610. In: de Martino, D., Silvotti, R., Solheim, JE., Kalytis, R. (eds) White Dwarfs. NATO Science Series, vol 105. Springer, Dordrecht. https://doi.org/10.1007/978-94-010-0215-8_20
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DOI: https://doi.org/10.1007/978-94-010-0215-8_20
Publisher Name: Springer, Dordrecht
Print ISBN: 978-1-4020-1364-5
Online ISBN: 978-94-010-0215-8
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