Department of Applied Mathematics, Faculty of Mathematics, Tabriz University, Tabriz, Islamic Republic of Iran
Abstract
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.
Rahimi Ardabili, M. (2003). LINEAR PULSATION CHARACTERISTICS
OF MIRA VARIABLE STARS. Journal of Sciences, Islamic Republic of Iran, 14(4), 363–365.
MLA
Rahimi Ardabili, M. "LINEAR PULSATION CHARACTERISTICS
OF MIRA VARIABLE STARS", Journal of Sciences, Islamic Republic of Iran, 14, 4, 2003, 363–365.
HARVARD
Rahimi Ardabili, M. (2003). 'LINEAR PULSATION CHARACTERISTICS
OF MIRA VARIABLE STARS', Journal of Sciences, Islamic Republic of Iran, 14(4), pp. 363–365.
CHICAGO
Rahimi Ardabili, M., "LINEAR PULSATION CHARACTERISTICS
OF MIRA VARIABLE STARS." Journal of Sciences, Islamic Republic of Iran, 14 4 (2003): 363–365,
VANCOUVER
Rahimi Ardabili M. LINEAR PULSATION CHARACTERISTICS
OF MIRA VARIABLE STARS. J. Sci. I. R. I. 2003;14(4):363–365.
Journal of Sciences, Islamic Republic of Iran