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Propagation of molecular outflows into inhomogeneous media

Corkery, Seán (2008) Propagation of molecular outflows into inhomogeneous media. Master of Science thesis, Dublin City University.

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Abstract

Molecular clouds have inhomogeneous density profiles and have been observed to be `clumpy' in nature, containing dense cores, rarefied filaments and cocoons. Energetic mass-ejection phenomena created during the gravitational collapse of dense cores are thought to be responsible for the molecular outflows that are observed in molecular clouds. Interactions between these molecular outflows and the inhomogeneous molecular clouds they encounter may cause changes in the observable characteristics of the outflows by affecting their velocity structure and morphology. Consequently, in this work, we aim to gain an understanding of the consequences of a relaxation of the usual assumption of a homogeneous molecular cloud or ambient medium, that is normally made in numerical simulations of molecular outflows. In particular, we simulate outflows propagating into inhomogeneous molecular clouds of decreasing density, i.e. outflows in the process of leaving their parent molecular clouds. We would expect such flows to appear severely truncated in CO emission maps, in comparison to their full flow extents. Using various prescriptions for inhomogeneous media to create more realistic density profiles, long duration numerical simulations are run. The simulations include the use of an improved cooling function the effects of which we describe. Standard observational methods are used for inferring the average outflow velocity and outflow age from the simulations. We examine the effects of the different density profiles on these key parameters and on the density structure, mass-velocity relations and length-to-width ratios that characterise the outflows.

Item Type:Thesis (Master of Science)
Date of Award:November 2008
Refereed:No
Supervisor(s):Downes, Turlough P.
Uncontrolled Keywords:Star formation; molecular outflows;
Subjects:Physical Sciences > Astronomy > Astrophysics
Mathematics
Computer Science > Computer simulation
DCU Faculties and Centres:DCU Faculties and Schools > Faculty of Science and Health > School of Mathematical Sciences
Use License:This item is licensed under a Creative Commons Attribution-NonCommercial-No Derivative Works 3.0 License. View License
Funders:Irish Research Council for Science Engineering and Technology, School of Mathematical Sciences, DCU, CosmoGrid (HEA PRTLI4 project)
ID Code:577
Deposited On:10 Nov 2008 12:12 by Turlough Downes. Last Modified 09 Dec 2011 12:03

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