Description of star formation in the context of cosmological large-scale structure formation
✍ Scribed by M. Hoeft; J.P. Mücket; P. Heide
- Publisher
- Elsevier Science
- Year
- 2001
- Tongue
- English
- Weight
- 132 KB
- Volume
- 688
- Category
- Article
- ISSN
- 0375-9474
No coin nor oath required. For personal study only.
📜 SIMILAR VOLUMES
This paper summarizeS the basic idea of coupling of density perturbation modes in Newtonian cosmology and the formation of primordial stars. The way of deriving the sccond-order differential equation governing the growth of two coupled adiabatic density perturbation modes in the matter era is brief
In cosmology numerical simulations of structure formation are now of central importance, as they are the sole instrument for providing detailed predictions of current cosmological models for a whole class of important constraining observations. These simulations are essentially molecular dynamics si
## Abstract The evolution of accretion disks and the formation of jets around super‐massive black holes are studied by 3‐D magnetohydrodynamic simulations. The previous studies of astrophysical jets have been concentrated on the effects of large‐scale magnetic fields permeating accretion disks. How