Abstract
Using our three-dimensional hydrodynamics code BTSPH (Binary Tree SPH; Kim et al. 1994), we have simulated the head-on collisions between two identical clouds with 8000 particles. As an initial cloud we take an isothermal polytropic sphere in hydrostatic equilibrium with an external medium. Following Nagasawa & Miyama (1987) we characterize the initial cloud by parameter A defined as A = (36π/125)[G3M2/c8 s]P ext, where M is the cloud mass, c s means the isothermal sound speed and P ext represents the external pressure. The collision conditions are fully described by the parameter A and the relative collision Mach number defined as M rel ≡ u rel/c s with u rel being the relative velocity of the two clouds. We have examined the collision outcomes for total 45 combinations of A and M rel.
Access this chapter
Tax calculation will be finalised at checkout
Purchases are for personal use only
References
Kim. W.-T., Hong, S. S., & Yun, H. S. 1994, JKAS, 27, 13
Nagasawa, M. & Miyama, S. M. 1987, Prog, of Theo. Phy., 78, 1250
Author information
Authors and Affiliations
Editor information
Editors and Affiliations
Rights and permissions
Copyright information
© 1999 Springer Science+Business Media Dordrecht
About this paper
Cite this paper
Kim, WT., Hong, S.S., Yoon, SC., Lee, S.M., Kim, J. (1999). Head-On Collisions of Isothermal Clouds. In: Miyama, S.M., Tomisaka, K., Hanawa, T. (eds) Numerical Astrophysics. Astrophysics and Space Science Library, vol 240. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-4780-4_37
Download citation
DOI: https://doi.org/10.1007/978-94-011-4780-4_37
Publisher Name: Springer, Dordrecht
Print ISBN: 978-94-010-6008-0
Online ISBN: 978-94-011-4780-4
eBook Packages: Springer Book Archive