LINEAR PULSATION CHARACTERISTICS OF MIRA VARIABLE STARS

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RAHIMI ARDABILI M.Y.

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Journal: Journal of Sciences, Islamic Republic of Iran Year:2003 | Volume:14 | Issue:4 Page(s): 363-365

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Information Journal Paper

Title

LINEAR PULSATION CHARACTERISTICS OF MIRA VARIABLE STARS

Author(s)

RAHIMI ARDABILI M.Y. | Issue Writer Certificate

Keywords

L.M.C.; MASS-LUMINOSITY RELATION; MIRA STARS; STELLAR PULSATIONQ4

Abstract

The linear adiabatic pulsation-periods of Mira variable stars have been derived. Approximately 2701†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 luminosityperiod- 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.

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APA: Copy

RAHIMI ARDABILI, M.Y.. (2003). LINEAR PULSATION CHARACTERISTICS OF MIRA VARIABLE STARS. JOURNAL OF SCIENCES ISLAMIC REPUBLIC OF IRAN, 14(4), 363-365. SID. https://sid.ir/paper/373011/en

Vancouver: Copy

RAHIMI ARDABILI M.Y.. LINEAR PULSATION CHARACTERISTICS OF MIRA VARIABLE STARS. JOURNAL OF SCIENCES ISLAMIC REPUBLIC OF IRAN[Internet]. 2003;14(4):363-365. Available from: https://sid.ir/paper/373011/en

IEEE: Copy

M.Y. RAHIMI ARDABILI, “LINEAR PULSATION CHARACTERISTICS OF MIRA VARIABLE STARS,” JOURNAL OF SCIENCES ISLAMIC REPUBLIC OF IRAN, vol. 14, no. 4, pp. 363–365, 2003, [Online]. Available: https://sid.ir/paper/373011/en

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