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Amplitude and Period Changes in the δ Sct Star AN Lyncis

Published online by Cambridge University Press:  12 April 2016

A.-Y. Zhou
A.-Y. Zhou*
Affiliation:
National Astronomical Observatories, CAS, Beijing 100012, China, e-mail:[email protected]

Abstract

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We report a study of time-dependent behaviour of the light variations in the δ Set star AN Lyn, based on an analysis of new time-series CCD observations and existing data. The amplitude of the main frequency increased from 1994 to 2000 at a rate of 0.006 mmag/yr. The light variation of AN Lyn can be explained currently by amplitude variability mixed with multiperiodic pulsation. With the extended data base, results on XX Cyg are also reported.

Type
Part 2.4. Delta Scuti Stars
Information
International Astronomical Union Colloquium , Volume 185: Radial and Nonradial Pulsations as Probes of Stellar Physics , 2002 , pp. 332 - 333
Copyright
Copyright © Astronomical Society of the Pacific 2002

References

Handler, G., et al. 2000, MNRAS, 318, 511 Google Scholar
Kiss, L.L., & Derekas, A. 2000, IBVS, No. 4950 Google Scholar
Rodríguez, E., et al. 1997a, A&A, 324, 959 (R97a)Google Scholar
Rodríguez, E., et al. 1997b, A&A, 328, 235 (R97b)Google Scholar