Parker, Nicholas D. and White, Glenn J.
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We have obtained a high resolution map of the 12CO J=3-2 emission in the vicinity of HH102 in the L1551 molecular outflow. The data reveal the presence of several bright clumps within the thin shell of low-velocity blue-shifted outflowing gas. There is evidence for further fragmentation in the clumps, as signified by the high derived excitation temperatures and low beam-filling factors. The region of peculiarly energetic activity asociated with HH102 concides with the projected location of impact of a radio jet from IRS56 with the dense ambient gas surrounding the outflow cavity.
|Item Type:||Conference Item|
|Copyright Holders:||1991 International Astronomical Union|
|Extra Information:||Fragmentation of Molecular Cluds and Star Formation
Proceedings of the 147th Symposium of the International Astronomical Union
Edited by E. Falgarone, F. Boulanger & G. Duvert
Kluwer Academic Publishers
|Academic Unit/Department:||Science > Physical Sciences|
|Interdisciplinary Research Centre:||Centre for Earth, Planetary, Space and Astronomical Research (CEPSAR)|
|Depositing User:||G. J. White|
|Date Deposited:||25 May 2012 08:59|
|Last Modified:||25 May 2012 21:49|
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