In this paper the lig-ht curves of long period M-type stars were analysed. The method used was that of the autocorrelation and supse- quent power spectrum analysis. Applying this method we obtain the ampli- tudes of the overtones espressed in that of the fundamental as unit. The relation betweeD log P and the relative intensity of the first overtone A (1) was studied. slope of the
Some indication who curve
obtained that foı the Pop 1 stars the log P — A (I) nıay be different from the one valid with the Pop II stars, but as yet the evidence is not conciusive.
Birincil Dil | İngilizce |
---|---|
Konular | Matematik |
Bölüm | Research Article |
Yazarlar | |
Yayımlanma Tarihi | 1 Ocak 1962 |
Gönderilme Tarihi | 1 Ocak 1962 |
Yayımlandığı Sayı | Yıl 1962 Cilt: 12 |
Communications Faculty of Sciences University of Ankara Series A1 Mathematics and Statistics.
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