Kelly, M.L and Macdonald, G.H. (1995) The Circumstellar of Lynds 379-IRSI. Astrophysics and Space Science, 224 (1-2). pp. 497-498. ISSN 0004-640X .
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12CO J=2-1 maps of L379 IRS1 show a molecular outflow seen almost end-on while C18O J=2-1 emission covers a smaller central region, tracing virially bound material deeper within the cloud. Continuum maps at 450, 800 and 1100µm all trace an identical double peaked arc west of IRS1 and VLA NH3 (1,1) & (2,2) integrated intensity maps reveal the same double-peaked structure. An identical velocity gradient is seen in12CO,13CO, C18O and NH3 (1,1) & (2,2) following the arc-like structure of the continuum emission.
|Uncontrolled keywords:||YSO - molecular cloud - L379 - IRAS 18265-1517|
|Subjects:||T Technology > TL Motor vehicles. Aeronautics. Astronautics|
|Divisions:||Faculties > Science Technology and Medical Studies > School of Physical Sciences > Centre for Astrophysics and Planetary Sciences|
|Depositing User:||P. Ogbuji|
|Date Deposited:||28 May 2009 18:08|
|Last Modified:||08 May 2012 10:14|
|Resource URI:||http://kar.kent.ac.uk/id/eprint/19644 (The current URI for this page, for reference purposes)|
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