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- W3103069898 abstract "Context.The high energies of protostellar jets, implied by recent observations of X-rays from such flows, came very much as a surprise. Inferred shock velocities are considerably higher than what was previously known, hence putting even larger energy demands on the driving sources of the jets. The statistics of X-ray emitting jets are still poor, yet a few cases exist which seem to imply a correlation between the presence of He I 1.0830 μm emission and X-ray radiation in a given source." @default.
- W3103069898 created "2020-11-23" @default.
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- W3103069898 date "2006-09-12" @default.
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- W3103069898 title "X-ray and He I 1.0830μm emission from protostellar jets" @default.
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- W3103069898 doi "https://doi.org/10.1051/0004-6361:20065990" @default.
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