The Bulletin of The Korean Astronomical Society (천문학회보)
- Volume 35 Issue 1
- /
- Pages.71.2-71.2
- /
- 2010
- /
- 1226-2692(pISSN)
Analysis of the North Galactic Pole region with FIMS
- Published : 2010.04.06
Abstract
Cooling hot gas sets a floor on the ionization level for diffuse gas in the ISM in general and the galactic halo. Many high galactic latitude sight lines, cooling hot gas is the dominant source of the ionization. Such sites are prime regions for the formation of both C IV and Si IV ions at a temperature of T~105K. To study of the ISM that have the 104.5~6K ionization state by ionization or photoionization by the collision, searching for the radiation energy that is emitted at far ultra violet range is required. In this paper, we report the analysis of NGP( North Galactic Pole,
Keywords