The Circumstellar of Lynds 379-IRSI

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 . (The full text of this publication is not available from this repository)

The full text of this publication is not available from this repository. (Contact us about this Publication)
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
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)
  • Depositors only (login required):