| |
 |
| Paper: |
Generation of Knots in a Randomly Pulsed Protostellar Jet: Synthesis of the X-ray Emission |
| Volume: |
448, 16th Cambridge Workshop on Cool Stars, Stellar Systems, and the Sun |
| Page: |
559 |
| Authors: |
Bonito, R.; Orlando, S.; Miceli, M.; Eislöffel, J.; Peres, G.; Favata, F. |
| Abstract: |
X-rays from protostellar jets have been discovered first in HH 2 and HH 154 and are now considered as a general feature of jets.
HH 154 is among the best studied X-ray emitting jet: up to now it is the only jet whose X-ray source proper motion has been measured. By observing this jet in X-rays, a complex morphology of the detected source has been revealed.
Here we discuss the results of modeling a randomly ejected pulsed jet traveling into an initially homogeneous medium. Our model allows us to directly compare the model predictions and the observations. |
|
|
|
|
|
