Use this URL to cite or link to this record in EThOS: http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.599430
Title: Hydrodynamical simulations of interstellar gas : from star-forming clouds to spiral arms
Author: Gittins, D.
Awarding Body: University of Cambridge
Current Institution: University of Cambridge
Date of Award: 2004
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Abstract:
This thesis presents numerical investigations of interstellar gas under various conditions. Discrete, pressure-bounded gas ‘cloudlets’ are modelled with Smoothed Particle Hydrodynamics (SPH) which is shown to reproduce accurately their properties and the outcomes of collisions between them. A simple model of a molecular cloud is investigated, consisting of a spherical ensemble of such cloudlets. This model dissipates its kinetic energy on a timescale controlled by the collision timescale. Distributed star formation does not result, and hierarchical mergers of cloudlets do not play a significant part, due to the high Mach number of collisions. A model gravitational potential for a spiral galaxy is introduced, and the interaction of large groups of cloudlets with this potential is investigated. Density and velocity structure are induced by the passage through a spiral arm. Comparisons to observed molecular clouds fail to reproduce the correct size-linewidth relation. The response of a uniform gaseous galactic disc to the spiral potential is investigated using two-dimensional SPH, a two-dimensional Eulerian code and a semi-analytical approach. Good agreement in the predicted location of spiral shocks is seen between all methods. Instability of spiral arms in open spirals is found, and possible formation mechanism of spur-like structure are discussed. The location of spiral shocks relative to the peaks of the stellar surface density is proposed as a new way to constrain the corotation radius in spiral galaxies. The potential form an N-body simulation of a galaxy is introduced and the response of the gaseous disc shows complex and rapidly changing structure. Observational implications for spatial galaxies are suggested.
Supervisor: Not available Sponsor: Not available
Qualification Name: Thesis (Ph.D.) Qualification Level: Doctoral
EThOS ID: uk.bl.ethos.599430  DOI: Not available
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