Internal shock model for microquasars
We present a model for the radio outbursts of microquasars based on the assumption of quasi-continuous jet ejection. The jets are 'lit up' by shock fronts traveling along the jets during outbursts. The shocks accelerate relativistic particles which emit the observed synchrotron radiation....
| Main Authors: | , , |
|---|---|
| Format: | Article |
| Language: | English |
| Published: |
2000.
|
| Subjects: | |
| Online Access: | Get fulltext |