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
M Rahimi Ardabili, "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