X-Ray Emission from Young Stellar Jets
Abstract
Jets from protostars and T Tauri stars define a separate and new class of X-ray sources. New evidence suggests that X-ray emission originates in microjets of several classical T Tauri stars. We summarize the present status of our search for jet-related X-ray emission and discuss physical implications for the jet gas.
- Publication:
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Protostellar Jets in Context
- Pub Date:
- 2009
- DOI:
- 10.1007/978-3-642-00576-3_41
- Bibcode:
- 2009ASSP...13..347G
- Keywords:
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- Physics