The Phillips relation of 'Normal' type Ia Supernovae
The use of Type Ia Supernovae (SNe Ia) as distance indicators relies on the calibration of their brightness using the observed property that brighter SNe have broader, slower light curves. Among possible causes are different masses of the progenitor white dwarfs or different opacities. We construct...
| 主要作者: | |
|---|---|
| 格式: | Conference item |
| 出版: |
2001
|