The interacting two winds model and a spherical density distribution function are introduced to study the dynamical and ionization structure of the planetary nebula IC 418. A fast wind with a mechanical luminousity 2/34×1034erg.s-1 of interacts with a super wind with a mass-loss rate of 2×10-5M(°)yr-1 and a velocity of 10 , and produces a dense and luminous medium. In this model, the expansion velocities of OI and HI lines are predicted to be 11 and 10.5kms-1 , respectively. The calculated dynamical time-scale 1033yr for the nebula is in good agreement with the evolution time of the central star after the interaction of the two winds. Our calculations give a luminosity 0.05M(°)of for the central star
J. Ghanbari, & A. Khesali, . (2020). A Model for the Dynamical and Ionization Structure of Planetary Nebula IC 418. Iranian Journal of Physics Research, 1(2), 103–109.
MLA
J. Ghanbari, & A. Khesali, . "A Model for the Dynamical and Ionization Structure of Planetary Nebula IC 418", Iranian Journal of Physics Research, 1, 2, 2020, 103–109.
HARVARD
J. Ghanbari, & A. Khesali, . (2020). 'A Model for the Dynamical and Ionization Structure of Planetary Nebula IC 418', Iranian Journal of Physics Research, 1(2), pp. 103–109.
CHICAGO
J. Ghanbari, & A. Khesali, , "A Model for the Dynamical and Ionization Structure of Planetary Nebula IC 418." Iranian Journal of Physics Research, 1 2 (2020): 103–109,
VANCOUVER
J. Ghanbari , A. Khesali . A Model for the Dynamical and Ionization Structure of Planetary Nebula IC 418. Iranian Journal of Physics Research. 2020;1(2):103–109 (In Persian).
