Chemodynamics is the appropriate treatment of the Interstellar Medium with its thermal and dynamical properties of various "phases" as well as of the stellar component in galaxy evolution. Furthermore, the chemical abundances of the gaseous and stellar components and their energetic and materialistic interactions are taken into account (see figure above).
For detailed information see:
- Hensler G.
The Chemo-dynamical Treatment of Galaxy Evolution
in "CNO in the Universe", eds. C. Charbonnel et al., 2003, ASP Conf. Ser. 304, 371 - Theis C., Burkert A. & Hensler G.
Chemo-dynamical Evolution of Massive Spherical Galaxies
A&A, 265, 465 (1992) - Samland M., Hensler G. & Theis C.
Modeling the Evolution of Disk Galaxies. I. Chemo-dynamical Method and a first Galaxy Model
1997, ApJ, 476, 544 - Rieschick A. & Hensler G.
Dynamical Processes, Element Mixing and Chemodynamical Cycles in Dwarf Galaxies
in Proc. III. Haro Conference "Cosmic Evolution and Galaxy Formation: Structure, Interactions, and Feedback", eds. J.Franco et al., San Francisco, 2000, ASP Conf. Ser., 215, 130 - Hensler G., Theis C. & Gallagher J.S.
Chemo-dynamical Evolution of Dwarf Ellipticals
2004, A&A, 426, 25
