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Rahimi Ardabili, M.Y.. (1382). LINEAR PULSATION CHARACTERISTICS OF MIRA VARIABLE STARS. , 14(4), 363-365.
M.Y. Rahimi Ardabili. "LINEAR PULSATION CHARACTERISTICS OF MIRA VARIABLE STARS". , 14, 4, 1382, 363-365.
Rahimi Ardabili, M.Y.. (1382). 'LINEAR PULSATION CHARACTERISTICS OF MIRA VARIABLE STARS', , 14(4), pp. 363-365.
Rahimi Ardabili, M.Y.. LINEAR PULSATION CHARACTERISTICS OF MIRA VARIABLE STARS. , 1382; 14(4): 363-365.

LINEAR PULSATION CHARACTERISTICS OF MIRA VARIABLE STARS

Journal of Sciences, Islamic Republic of Iran
مقاله 9، دوره 14، شماره 4، اسفند 2003، صفحه 363-365    اصل مقاله (244 K)
نوع مقاله: Original Paper
نویسنده
M.Y. Rahimi Ardabili*
Department of Applied Mathematics, Faculty of Mathematics, Tabriz University, Tabriz, Islamic Republic of Iran
چکیده
The linear adiabatic pulsation-periods of Mira variable stars have been derived. Approximately 2701[1]models were calculated for M = 0.7 MΘ to 2 MΘ stars with radii from 180 RΘ to 340 RΘ and luminosities from 2800 LΘ to 10,000 LΘ. The chemical composition of all models is (X,Z) = (0.7,0.02). From the result of this study, linear relations on Luminosity-Period-Mass relationship and luminosity-period-radius-mass relationship have been derived for the fundamental mode. The relation has been tested on a recent data set of Mira stars in the LMC.



1 Models of various computational input are available through the author.
کلیدواژه‌ها
L.M.C؛ Mass-luminosity relation؛ Mira stars؛ Stellar pulsation
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