LINEAR PULSATION CHARACTERISTICS OF MIRA VARIABLE STARS

نویسنده

  • M.Y. Rahimi Ardabili Department of Applied Mathematics, Faculty of Mathematics, Tabriz University, Tabriz, Islamic Republic of Iran
چکیده مقاله:

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.

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عنوان ژورنال

دوره 14  شماره 4

صفحات  363- 365

تاریخ انتشار 2003-12-01

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