Astronomy and Astrophysics – Astronomy
Scientific paper
Oct 2005
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005asthe..98..627n&link_type=abstract
The Astronomical Herald (ISSN 0374-2466), Vol. 98, No. 10, p. 627 - 634 (2005)
Astronomy and Astrophysics
Astronomy
Algol Systems, Photometry
Scientific paper
Many primary stars in the Algol-type systems are recently recognized as pulsating stars. Although the traditional classification scheme indicates that such stars are the δ Sct stars, there are some doubts in this classification. It is proposed that in such a system the oscillation in the primary component is strongly affected by the mass transfer from the secondary to the primary. We have been observing such variables, especially focusing on RZ Cas, with the 60 cm telescope in the Nishi-Harima Astronomical Observatory. In this article, we will report our recent results. We will also present photometric studies of the eclipsing binaries by amateur observers using portable telescopes.
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