Structure in star forming regions

Stars form in clumpy, highly substructured environments. In this thesis I set up N-body simulations of substructured star forming regions and investigate the impact that the substructure has on the survival of the star forming regions. I also present a broad range of methods used in other fields to...

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Bibliographic Details
Main Author: Lee, Pawel
Other Authors: Goodwin, Simon
Published: University of Sheffield 2016
Subjects:
500
Online Access:http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.682318
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spelling ndltd-bl.uk-oai-ethos.bl.uk-6823182017-10-04T03:25:48ZStructure in star forming regionsLee, PawelGoodwin, Simon2016Stars form in clumpy, highly substructured environments. In this thesis I set up N-body simulations of substructured star forming regions and investigate the impact that the substructure has on the survival of the star forming regions. I also present a broad range of methods used in other fields to quantify and identify structure. I discuss their strengths and shortcomings and assess their suitability for use in astronomical contexts. I use the Q and Λ methods to compare the distributions of class I and class II sources in observed star forming regions to learn more about the dynamical evolution of systems and infer whether they are bound or unbound.500University of Sheffieldhttp://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.682318http://etheses.whiterose.ac.uk/12395/Electronic Thesis or Dissertation
collection NDLTD
sources NDLTD
topic 500
spellingShingle 500
Lee, Pawel
Structure in star forming regions
description Stars form in clumpy, highly substructured environments. In this thesis I set up N-body simulations of substructured star forming regions and investigate the impact that the substructure has on the survival of the star forming regions. I also present a broad range of methods used in other fields to quantify and identify structure. I discuss their strengths and shortcomings and assess their suitability for use in astronomical contexts. I use the Q and Λ methods to compare the distributions of class I and class II sources in observed star forming regions to learn more about the dynamical evolution of systems and infer whether they are bound or unbound.
author2 Goodwin, Simon
author_facet Goodwin, Simon
Lee, Pawel
author Lee, Pawel
author_sort Lee, Pawel
title Structure in star forming regions
title_short Structure in star forming regions
title_full Structure in star forming regions
title_fullStr Structure in star forming regions
title_full_unstemmed Structure in star forming regions
title_sort structure in star forming regions
publisher University of Sheffield
publishDate 2016
url http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.682318
work_keys_str_mv AT leepawel structureinstarformingregions
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