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The Circumstellar of Lynds 379-IRSI

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: 16 Nov 2021 09:57 UTC
Resource URI: https://kar.kent.ac.uk/id/eprint/19644 (The current URI for this page, for reference purposes)

University of Kent Author Information

Macdonald, G.H..

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