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S. De Ruyter, H. Van Winckel, C. Domind, et al., “Strong Dust Processing in Circum Stellar Disk around RV Tauri Stars,” Astronomy and Astrophysics Journal, Vol. 435, 2005, pp. 161-166.

has been cited by the following article:

• TITLE: The Mechanism of Interacting Stellar Winds beyond Red Giant Branch

  AUTHORS: Sundus A. Abdullah Albakri, Sinan H. Ali

  KEYWORDS: Nebulae; Stars; Evolution; Mass Loss

  JOURNAL NAME: International Journal of Astronomy and Astrophysics, Vol.3 No.4, October 9, 2013

  ABSTRACT: The dynamical processes of the interaction of slow wind beyond Red Giant phase with fast wind of central star of nebula are evaluated. The mechanism of interaction stellar wind model (ISW) is found to be responsible for producing a relatively dense shell of gas which increases in mass and radius at a constant rate. Both slow wind and superwind are assumed to be time independent and radial density is calculated at initial time to ~ 60 yrs with the fast wind velocity (v ≈ 1000 km/s). The results showed that, at the outer rim of super wind region, a small density hump appears due to the relative velocity between slow winds and central star winds, in a good agreement with the previous models. The dynamical requirements of the observed expansion of planetary nebulae can be satisfied by the mechanism of interacting stellar wind model with reasonable mass loss rate from central star.