. 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
Bonito, R., Orlando, S., Miceli, M., Eislöffel, J., Peres, G., Favata, F. (2011). Generation of Knots in a Randomly Pulsed Protostellar Jet: Synthesis of the X-ray Emission. In 16TH CAMBRIDGE WORKSHOP ON COOL STARS, STELLAR SYSTEMS AND THE SUN (pp. 559-563). Astronomical Society of the Pacific.
Generation of Knots in a Randomly Pulsed Protostellar Jet: Synthesis of the X-ray Emission
BONITO, Rosaria
;MICELI, Marco;PERES, Giovanni;
2011-01-01
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
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