A. Abdullah, S., A. Abutaib, M., A. Ali, N., T.Jiaad, B. (2012). THE DYNAMIC EVOLUTION OF THE SHELL NEBULAE BY USING INTERACTING WIND MODEL. Alustath, 0(0), 24-30.
Sundus A. Abdullah; Mohamed A. Abutaib; Nathera A. Ali; Behaa T.Jiaad. "THE DYNAMIC EVOLUTION OF THE SHELL NEBULAE BY USING INTERACTING WIND MODEL". Alustath, 0, 0, 2012, 24-30.
A. Abdullah, S., A. Abutaib, M., A. Ali, N., T.Jiaad, B. (2012). 'THE DYNAMIC EVOLUTION OF THE SHELL NEBULAE BY USING INTERACTING WIND MODEL', Alustath, 0(0), pp. 24-30.
A. Abdullah, S., A. Abutaib, M., A. Ali, N., T.Jiaad, B. THE DYNAMIC EVOLUTION OF THE SHELL NEBULAE BY USING INTERACTING WIND MODEL. Alustath, 2012; 0(0): 24-30.

THE DYNAMIC EVOLUTION OF THE SHELL NEBULAE BY USING INTERACTING WIND MODEL

Basic Education College Magazine For Educational and Humanities Sciences
Article 1, Volume 0, Issue 0, January 2018, Pages 24-30
Authors
Sundus A. Abdullah; Mohamed A. Abutaib; Nathera A. Ali; Behaa T.Jiaad
Abstract
Planetary Nebulae (PN) are astronomical objects made up primarily of gaseous materials. A planetary nebulae are an emission nebulae consisting of an expanding glowing shell of ionized gas ejected during the Asymptotic Giant Branch (AGB) phase. of certain types of stars late in their life. late in their life
Keywords
THE DYNAMIC EVOLUTION OF THE SHELL NEBULAE BY USING INTERACTING WIND MODEL
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