Article contents
Modeling the Local Bubble Using Multiple Supernova Remnants
Published online by Cambridge University Press: 12 April 2016
Abstract
We have modeled the Local Bubble (LB) using a one-dimensional hydrocode (ODIN) that can simulate multiple supernova remnants, with non-equilibrium ion evolution and dust. Our model assumes that the local interstellar medium was a cool (104 K) gas approximately 5-10 Myr ago; it was then disturbed by 2 or 3 supernovae exploding within 20-30 pc of each other over a period of 2-4 million years. The LB is the leftover hot gas from these explosions. The model predicts the x-ray emission from such a bubble, as well as ionic abundances for hot gas ions such as O VI. These are compared to the soft x-ray data from the Wisconsin all-sky survey and the ROSAT PSPC.
- Type
- Part III Observations and Modeling of the Local Bubble and the SXRB
- Information
- International Astronomical Union Colloquium , Volume 166: The Local Bubble and Beyond , 1997 , pp. 133 - 136
- Copyright
- Copyright © Springer-Verlag 1998
References
- 1
- Cited by