Kelly, M.L., Macdonald, G.H. (1995) The Circumstellar of Lynds 379-IRSI. Astrophysics and Space Science, 224 (1-2). pp. 497-498. ISSN 0004-640X. (doi:10.1007/BF00667923) (The full text of this publication is not currently available from this repository. You may be able to access a copy if URLs are provided) (KAR id:19644)
| The full text of this publication is not currently available from this repository. You may be able to access a copy if URLs are provided. | |
| Official URL: http://dx.doi.org/10.1007/BF00667923 |
Abstract
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.
| Item Type: | Article |
|---|---|
| DOI/Identification number: | 10.1007/BF00667923 |
| Uncontrolled keywords: | YSO - molecular cloud - L379 - IRAS 18265-1517 |
| Subjects: | T Technology > TL Motor vehicles. Aeronautics. Astronautics |
| Divisions: | Divisions > Division of Natural Sciences > Physics and Astronomy |
| Depositing User: | P. Ogbuji |
| Date Deposited: | 28 May 2009 18:08 UTC |
| Last Modified: | 05 Nov 2024 09:56 UTC |
| Resource URI: | https://kar.kent.ac.uk/id/eprint/19644 (The current URI for this page, for reference purposes) |
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