Classification of Mira variables based on visual light curve shape

Details Classification of Mira variables based on visual light curve shape Classification of Mira variables based on visual light curve shape

Apr 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988a%26as...73..181v&link_type=abstract

Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 73, no. 1, April 1988, p. 181-194.

Astronomy and Astrophysics

Astrophysics

8

Astronomical Photometry, Cool Stars, Light Curve, Mira Variables, Astronomical Catalogs, Histograms

Scientific paper

The paper presents classifications of 368 Mira variables of M, S and C spectral classes based on the shape of their visual light curve. The classification is esentially based on Ludendorff's (1928) scheme and the light curves used are mainly from the compilation of Campbell (1955). The distribution of light curves over period, mean amplitude, light curve asymmetry factor, period variability, and spectral class at maximum is discussed.

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