eprintid: 29009
rev_number: 13
eprint_status: archive
userid: 5309
dir: disk0/00/02/90/09
datestamp: 2020-11-03 08:19:07
lastmod: 2020-11-05 13:19:37
status_changed: 2020-11-03 08:19:07
type: doctoralThesis
metadata_visibility: show
creators_name: Jeffreson, Sarah May Rose
title: Giant molecular clouds under the influence of the galactic environment
subjects: ddc-520
divisions: i-130001
adv_faculty: af-13
abstract: The vast majority of star formation in galaxies begins in cold, dense, fractally-structured reservoirs of molecular hydrogen known as giant molecular clouds. The instantaneous
properties of these clouds and the time-scales on which they evolve can therefore be built up into models of the empirical properties of galactic-scale star formation, and so can be used to understand this process. In this thesis, we first propose a simple analytic framework to quantify the expected variation in the physical properties and lifetimes of giant molecular clouds in response to changes in their galactic-dynamical environments, finding that they vary within a fundamental parameter space spanned by the orbital angular velocity of the host galaxy, the degree of galactic shearing, the gravitational stability, and the mid-plane hydrostatic pressure. We then explore this parameter space using a set of high-resolution numerical simulations of Milky Way-like galaxies. Due to their high densities and pressures relative to the galactic mid-plane, we find that giant molecular clouds in Milky Way-like galaxies are self-gravitating and decoupled from galactic dynamics, by contrast to their lower-density progenitor clouds of atomic gas, which display systematic, galactic-dynamical variations. Finally, we analyse the full evolutionary history of each simulated cloud population as a function of the cloud spatial scale. Across all Milky Way-like environments, we find that the lifetimes of self-gravitating clouds decrease with their spatial scale below the scale-height of the thin gas disc of the galaxy, and converge to the disc crossing time at its scale-height.
date: 2020
id_scheme: DOI
id_number: 10.11588/heidok.00029009
ppn_swb: 173796922X
own_urn: urn:nbn:de:bsz:16-heidok-290091
date_accepted: 2020-10-28
advisor: HASH(0x55fc36c59be8)
language: eng
bibsort: JEFFRESONSGIANTMOLEC2020
full_text_status: public
place_of_pub: Heidelberg
citation:   Jeffreson, Sarah May Rose  (2020) Giant molecular clouds under the influence of the galactic environment.  [Dissertation]     
document_url: https://archiv.ub.uni-heidelberg.de/volltextserver/29009/1/Jeffreson-Sarah-2020.pdf