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Ross 548
Ross 548 is a variable white dwarf star of the DAV type. It was found to be variable in 1970;〔(High-Frequency Stellar Oscillations. VI. R548, a Periodically Variable White Dwarf ), Barry M. Lasker and James E. Hesser, ''Astrophysical Journal'' 163 (February 1971), pp. L89–L93.〕 in 1972, it was given the variable star designation ZZ Ceti,〔(58th Name-List of Variable Stars ), B. V. Kukarkin, P. N. Kholopov, N. P. Kukarkina, N. B. Perova, ''Information Bulletin on Variable Stars'', #717, September 21, 1972.〕 which also refers to the entire class of DAV variable white dwarfs.〔(Physics of white dwarf stars ), D. Koester and G. Chanmugam, ''Reports on Progress in Physics'' 53 (1990), pp. 837–915.〕, pp. 891, 895. ==See also==
*ZZ Ceti variable
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