Volume 385, Number 3, April III 2002
|Page(s)||793 - 801|
|Section||Cosmology (including clusters of galaxies)|
|Published online||15 April 2002|
Search for second overtone mode Cepheids in Magellanic Clouds*
II. Characteristics of second overtone mode pulsations
Osservatorio Astronomico di Brera, via E. Bianchi 46, 23807 Merate, Italy
Corresponding author: E. Antonello, email@example.com
Accepted: 17 January 2002
The analysis of CCD observations of ten new suspected second overtone mode Cepheids in the SMC does not confirm the nature of such stars; most of them appear to be first overtone mode Cepheids. A careful analysis of the OGLE best second overtone mode candidates and of the second overtone component of double mode Cepheids in SMC and LMC has been performed in order to clarify the possible effects of a resonance between pulsation modes. There are some indications that such a resonance is indeed operating in these pulsators. A brief discussion of the effects of blending on the light curve shape is also reported, and the usefulness of the Fourier parameters as mode discriminators is discussed.
Key words: stars: oscillations / stars: variables: Cepheids / galaxies: Magellanic Clouds
© ESO, 2002
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.