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- W2079894197 abstract "A high-resolution (|$0.6 {rm arcsec pixel}^{-1}$|), narrow-band, |${rm H}_2 v=1-0 {rm S}(1)$| image of the high-velocity CO outflow in L1448 reveals a remarkable jet-like structure. The coincidence of this |${rm H}_2$| jet with the CO bipolar outflow implies a close association between the two phenomena. The |${rm H}_2$| jet comprises a series of knots, and three bow-shaped features equally spaced along the jet length, which we associate with the sporadic nature of this outflow. K-band imaging of the source also shows a conical reflection nebula extending towards the |${rm H}_2$| jet structure, whilst maps in |${rm HCO}^+ J=3-2$| and |${rm CS} J=5-4$| show two peaks, one towards the source of the |${rm H}_2$| jet and CO outflow, and the other towards the infrared source IRS 3 situated to the north of this region. Together these observations suggest that the |${rm H}_2$| jet represents the shock interface between a stellar wind from the L1448-mm source and the surrounding molecular gas, although the CO outflow is not thought to be dependent on this interaction." @default.
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- W2079894197 date "1994-02-15" @default.
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- W2079894197 title "Submillimetre and near-infrared observations of L1448: a curving Formula jet with multiple bow shocks" @default.
- W2079894197 doi "https://doi.org/10.1093/mnras/266.4.933" @default.
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