The objectives of this study is, by combining ASCA and XTE data, to search for a non thermal emission in the spectrum of Kepler's supernova remnant and to derive a consistent model of the thermal emission by using hydrodynamical models coupled to non equilibrium ionization calculation.
β¦ LIBER β¦
A new galactic supernova remnant in the direction of G69.7+1.0
β Scribed by K. Yoshita; E. Miyata; H. Tsunemi
- Publisher
- John Wiley and Sons
- Year
- 1999
- Tongue
- English
- Weight
- 136 KB
- Volume
- 320
- Category
- Article
- ISSN
- 0004-6337
No coin nor oath required. For personal study only.
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