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A&A Supplement Ser., Vol. 124, July 1997, 143-151
Received September 13; accepted November 16, 1996
M.O. Mennessier
, H. Boughaleb
,
and J.A. Mattei
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Université Montpellier II, Groupe de Recherche en
Astronomie et Astrophysique du Languedoc, Unité associée au CNRS,
F-34095 Montpellier Cedex 5, France
American Association of Variable Star Observers,
25 Birch Street, Cambridge, Massachusetts 02138-1205, U.S.A.
Université des Sciences El Jadida, Maroc
Using 75 years of AAVSO data, mean light curve parameters
of a sample of 355 long period M, S, and C mira and
semi-regular variable stars are investigated. We present
a classification of the light curves of LPVs into 6 distinct
groups. Combining this classification with IRAS colors
makes it possible to distinguish oxygen-rich from
carbon-rich miras.
keywords: stars: AGB, post-AGB -- methods: data analysis -- stars: carbon -- stars: variables