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Photometric Detection of Low-Order Nrp in Be Stars

Published online by Cambridge University Press:  12 April 2016

K. Pavlovski ,
Ž. Ružić  and
V. Vujnović
K. Pavlovski
Affiliation:
Hvar Observatory, Zagreb University, Kačićeva 26, 41000 Zagreb, Croatia
Ž. Ružić
Affiliation:
Hvar Observatory, Zagreb University, Kačićeva 26, 41000 Zagreb, Croatia
V. Vujnović
Affiliation:
Hvar Observatory, Zagreb University, Kačićeva 26, 41000 Zagreb, Croatia

Abstract

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Period analysis of Be stars 28 Cyg and EW Lac has shown that their photometric variations are multiperiodic. Dominant periods have counterpart in low-order NRP modes identified in the independent line profile studies.

Type
VIII. Asteroseismology: observation
Information
International Astronomical Union Colloquium , Volume 137: Inside the Stars , 1993 , pp. 724 - 726
Copyright
Copyright © Astronomical Society of the Pacific 1993

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