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Dissertations / Theses on the topic 'Cluster formation'

Author: Grafiati

Published: 4 June 2021

Last updated: 25 July 2025

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1

Dale, J. E. "Feedback in star cluster formation." Thesis, University of Cambridge, 2004. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.598249.

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Massive stars emit strong fluxes of ionising radiation and their dynamical impact on their natal clusters is expected to be severe. The outflows generated expel residual gas from the cluster and can potentially gravitationally disrupt it. The loss of its reserves of molecular gas also prevents the cluster forming more stars. Star-formation and star cluster evolution cannot be fully understood without a proper treatment of feedback. I present a novel technique I have developed to allow the inclusion of the effects of ionising radiation in smoothed particle hydrodynamics (SPH) simulations of sta

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2

Bailey, Philip John. "Carbide formation and cluster build-up reactions in ruthenium carbonyl cluster chemistry." Thesis, University of Cambridge, 1990. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.335689.

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3

Bergman, Edward M., and Patrick Lehner. "Industrial cluster formation in European regions. U.S. cluster templates and Austrian evidence." Institut für Wirtschaftsgeographie, Abt. Stadt- und Regionalentwicklung, WU Vienna University of Economics and Business, 1998. http://epub.wu.ac.at/748/1/document.pdf.

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The paper will be organized in the following manner. We first provide a concise review of how industrial trade clusters were developed from available I/O coefficients (see box), including how regional industrial data may be embedded within their "templates". Second, we will review the steps taken, using available industrial concordances, that permit regional data from other advanced national industrial systems to be embedded within these templates. Third, we will illustrate the results of applying the U.S. template for the motor vehicle industrial trade cluster to regions in both Austria and N

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4

Harris, William E., Stephanie M. Ciccone, Gwendolyn M. Eadie, et al. "GLOBULAR CLUSTER SYSTEMS IN BRIGHTEST CLUSTER GALAXIES. III. BEYOND BIMODALITY." IOP PUBLISHING LTD, 2017. http://hdl.handle.net/10150/622870.

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We present new deep photometry of the rich globular cluster (GC) systems around the Brightest Cluster Galaxies UGC 9799 (Abell 2052) and UGC 10143 (Abell 2147), obtained with the Hubble Space Telescope (HST) ACS and WFC3 cameras. For comparison, we also present new reductions of similar HST/ACS data for the Coma supergiants NGC 4874 and 4889. All four of these galaxies have huge cluster populations (to the radial limits of our data, comprising from 12,000 to 23,000 clusters per galaxy). The metallicity distribution functions (MDFs) of the GCs can still be matched by a bimodal-Gaussian form whe

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5

Chen, Bo-Gaun. "Cluster formation in supersonic beams of dense fluids." Doctoral thesis, Humboldt-Universität zu Berlin, Mathematisch-Naturwissenschaftliche Fakultät, 2015. http://dx.doi.org/10.18452/17441.

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Mit zeitaufgelöster Massenspektrometrie untersuchen wir die Winkelverteilung von Kohlendioxid-Monomeren bei der Streuung von Kohlendioxid-Clustern an einer Si(111)/Siliciumdioxid-Oberfläche unter Ultrahochvakuum-Bedingungen. Die präsen- tierten Studien decken eine große Breite der Clustergrößen, , 1,000 < N < 200,000 Moleküle pro Partikel, ab. Dabei liegt der Fokus auf dem Einfluss der Ausgangsentropie, die durch eine präzise Einstellung des Ausgangsdruckes und der Düsentemperatur realisiert wurde. Es zeigt sich, daß die Streuverteilung direkt den Expansionspfad widerspiegelt, wodurch eine Unt

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6

Strader, Jay. "Extragalactic globular cluster subpopulations and galaxy formation /." Diss., Digital Dissertations Database. Restricted to UC campuses, 2007. http://uclibs.org/PID/11984.

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7

Sacilotto, Cintia Kulzer. "Industrial cluster relocation : cluster formation, development and technological change in the destination region." Thesis, University of Oxford, 2017. http://ora.ox.ac.uk/objects/uuid:22ee5a2d-ea95-4c58-941a-5e6385e03f1a.

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This dissertation presents the first systematic study on cluster relocation, providing a non- random and dynamic analysis of firm relocations. Seeking to contribute to the understanding of cluster relocations and their consequences for the destination region, I explore the process and determinants of a particular cluster relocation and investigate the growth and maintenance of the new cluster through the enhancement of its supplier base, the diffusion of innovations, and advances in technological change. I analyse the differences between first and late mover firms in the process of cluster rel

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8

Hohertz, Jeremy D. "Formation of a globular cluster via gravitational capture." Oxford, Ohio : Miami University, 2008. http://rave.ohiolink.edu/etdc/view?acc%5Fnum=miami1217352629.

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9

Canning, Rebecca Elizabeth Ann. "Star and filament formation in brightest cluster galaxies." Thesis, University of Cambridge, 2012. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.610523.

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10

Santoro, Fernando. "Semi analytical simulations of primordial star cluster formation." Thesis, University of Sussex, 2003. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.288843.

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11

Heays, Katherine Grace. "Cluster formation and stream-bed armouring: a photogrammetric study." Thesis, University of Auckland, 2012. http://hdl.handle.net/2292/13048.

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Clusters are a self organising structures commonly found in natural rivers. They play an important role in river bed dynamics by providing habitat and increasing bed stability. The aim of the present study was to investigate the development of naturally formed cluster microforms from a flattened bed of graded gravel at constant flow rate. The study was laboratory based, and used photogrammetry to observe the behaviour of well graded, cohesionless sediment at flood flow conditions as clusters formed, evolved and disintegrated. Focus was primarily on the cluster formation and sediment move

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12

Cho, Jaeil. "Globular cluster systems and their implications of galaxy formation." Thesis, Durham University, 2008. http://etheses.dur.ac.uk/2427/.

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In this thesis the spectroscopic and photometric results of the Galactic and extragalactic globular clusters are presented. And their implications on galaxy formation have been investigated. Integrated spectroscopy with a high resolution of 24 Galactic globular clusters were obtained using the Isacc Newton Telescope, from which 21 line indices were carefully measured and calibrated. By comparing with recent simple stellar population models (Thomas et al. 2003 and Lee & Worthey 2005), it is confirmed that Galactic globular clusters are old (~10- 12 Gyr). There is a discrepancy between the t

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13

Fensch, Jérémy. "Star and stellar cluster formation in gas-dominated galaxies." Thesis, Sorbonne Paris Cité, 2017. http://www.theses.fr/2017USPCC207/document.

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Nous étudions la formation d’étoiles et d’amas d’étoiles dans les galaxies dominées par le gaz. Ce terme réfère en premier lieu aux galaxies de l’époque du pic de formation d’étoiles dans l’histoire de l’Univers, qui s’est déroulé vers z ~ 2, mais aussi à leurs analogues locaux, les galaxies naines de marées. En premier lieu, en utilisant des simulations numériques, nous montrons que les galaxies massives typiques de z=2, avec une fraction de gaz d’environ 50%, forment des structures gazeuses massives (10**7-8 masses solaires) et liées gravitationnellement, appelées grumeaux dans la suite. Ces

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Rudick, Craig S. "The Formation and Evolution of Intracluster Light: Simulations and Observations." Case Western Reserve University School of Graduate Studies / OhioLINK, 2011. http://rave.ohiolink.edu/etdc/view?acc_num=case1282831433.

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15

Cooke, Elizabeth A. "How to build a cluster : the formation and evolution of galaxies in high-redshift clusters and protoclusters." Thesis, University of Nottingham, 2016. http://eprints.nottingham.ac.uk/35454/.

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High redshift galaxy protoclusters are the precursors of today’s massive clusters; the sites of formation of the most massive galaxies in the present-day Universe. By studying these immature structures we can directly analyse the formation of galaxies in the densest environments without relying on extrapolations from low redshift. Finding protoclusters is challenging due to the need for very wide and deep surveys. Radio-loud active galactic nuclei (RLAGN) have been shown to preferentially reside in overdense environments at z > 1. By using these bright radio sources as beacons, protoclusters m

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16

Adamo, A., J. E. Ryon, M. Messa, et al. "Legacy ExtraGalactic UV Survey with The Hubble Space Telescope: Stellar Cluster Catalogs and First Insights Into Cluster Formation and Evolution in NGC 628." IOP PUBLISHING LTD, 2017. http://hdl.handle.net/10150/624449.

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We report the large effort that is producing comprehensive high-level young star cluster (YSC) catalogs for a significant fraction of galaxies observed with the Legacy ExtraGalactic UV Survey (LEGUS) Hubble treasury program. We present the methodology developed to extract cluster positions, verify their genuine nature, produce multiband photometry (from NUV to NIR), and derive their physical properties via spectral energy distribution fitting analyses. We use the nearby spiral galaxy NGC 628 as a test case for demonstrating the impact that LEGUS will have on our understanding of the formation

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17

Lin, Pei. "First-principles calculations of helium cluster formation in palladium tritides." Diss., Georgia Institute of Technology, 2010. http://hdl.handle.net/1853/41103.

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The accumulation of helium atoms in metals or metal tritides is known to result in the formation of helium bubbles in the lattice and to cause degradation of the material. Helium is introduced either through neutron transmutation reaction or via the radioactive decay of tritium. We have performed first-principles calculations of interstitial helium inside Pd and Pd tritide using density functional theory (DFT) and the projector augmented-wave (PAW) method within the generalized gradient approximation (GGA). We model the growth process of an interstitial helium cluster and find that when the si

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18

Corbett, Jennifer Leontine. "Sodium-cluster complexes : probability of formation, stability and mass spectra." Thesis, University of British Columbia, 2012. http://hdl.handle.net/2429/41966.

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Accurate knowledge of aerosol size and composition is important for the understanding of their effects on both the atmosphere and the health of those who inhale them. Ultrafine aerosols (0.25 nm to 10 nm radius) and small clusters (2 molecules to 0.25 nm radius) can only be detected down to radii of a few nanometers and no chemical information is provided. A photoion spectrometer was previously built and is used to dope clusters and ultrafine aerosols with Na atoms. The subsequent Na-cluster complexes are then ionized by a UV laser. This technique is currently believed to be the softest ioniza

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19

Thomas, Claire F. "Environmental dependence of star formation in field and cluster galaxies." Thesis, Liverpool John Moores University, 2006. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.439066.

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20

Akizuki, Makoto. "Gas Cluster Ion-Solid Surface Interaction and Thin Film Formation." Kyoto University, 1999. http://hdl.handle.net/2433/181783.

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21

Haack, Alexander [Verfasser]. "Theoretical Investigations on Cluster Formation in Mass Spectrometry / Alexander Haack." Wuppertal : Universitätsbibliothek Wuppertal, 2020. http://d-nb.info/1207005800/34.

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22

Shim, Young Hak. "Design of a cluster analysis heuristic for the configuration and capacity management of manufacturing cells." Diss., Texas A&M University, 2003. http://hdl.handle.net/1969.1/5905.

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This dissertation presents the configuration and capacity management of manufacturing cells using cluster analysis. A heuristic based on cluster analysis is developed to solve cell formation in cellular manufacturing systems (CMS). The clustering heuristic is applied for cell formation considering processing requirement (CFOPR) as well as various manufacturing factors (CFVMF). The proposed clustering heuristic is developed by employing a new solving structure incorporating hierarchical and non-hierarchical clustering methods. A new similarity measure is constructed by modifying the Jarccard s

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23

Messa, M., A. Adamo, G. Östlin, et al. "The young star cluster population of M51 with LEGUS – I. A comprehensive study of cluster formation and evolution." OXFORD UNIV PRESS, 2018. http://hdl.handle.net/10150/626277.

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Recently acquired WFC3 UV (F275W and F336W) imaging mosaics under the Legacy Extragalactic UV Survey (LEGUS), combined with archival ACS data of M51, are used to study the young star cluster (YSC) population of this interacting system. Our newly extracted source catalogue contains 2834 cluster candidates, morphologically classified to be compact and uniform in colour, for which ages, masses and extinction are derived. In this first work we study the main properties of the YSC population of the whole galaxy, considering a mass-limited sample. Both luminosity and mass functions follow a power-la

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24

Nuur, Cali. "Cluster Dynamics and Industrial Policy in Peripheral Regions : a study of cluster formation as a local development process." Doctoral thesis, Stockholm : Department of Industrial Economics and Management, Royal Institute of Technology : Arbetslivsinstitutet, 2005. http://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-475.

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25

Usui, Hiroaki. "IONIZED CLUSTER BEAM TECHNIQUES: Formation of Cluster Beams by Vaporized Solid Materials and Their Applications to Film Depositions." Kyoto University, 1987. http://hdl.handle.net/2433/74708.

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26

Tsai, Chao-Wei. "Star cluster formation in the nuclear regions of nearby spiral galaxies." Diss., Restricted to subscribing institutions, 2009. http://proquest.umi.com/pqdweb?did=1997620851&sid=1&Fmt=2&clientId=1564&RQT=309&VName=PQD.

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27

Perrett, Kathryn. "The globular cluster system of M31, keys to its formation history." Thesis, National Library of Canada = Bibliothèque nationale du Canada, 2001. http://www.collectionscanada.ca/obj/s4/f2/dsk3/ftp05/NQ63443.pdf.

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28

Wang, Yan. "Chinese entrepreneurship and cluster formation : multi-case studies from east China." Thesis, University of Central Lancashire, 2011. http://clok.uclan.ac.uk/3718/.

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Cluster is not a new phenomenon, having existed in different forms for a long time. Although a large amount of work has been dedicated to cluster research (Marshall, 1920; Krugman, 1995; Schmitz 1997; Porter, 1998; Wilson and Popp, 2003), there is still a lack of convincing explanations as to how and why clusters are created. Reviewing the different definitions of ‘cluster’ from previous studies, produces the interesting finding that most of the cluster definitions neglect one key element – the ‘actor’ – that is, the individuals who are involved in the process of founding new businesses that g

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29

SHAH, VIVEK. "PARALLEL CLUSTER FORMATION FOR SECURED COMMUNICATION IN WIRELESS AD HOC NETWORKS." University of Cincinnati / OhioLINK, 2004. http://rave.ohiolink.edu/etdc/view?acc_num=ucin1097709696.

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30

Tirumalai, Nakul. "LCPlace: A Novel VLSI Placement Methodology based on large cluster formation." University of Cincinnati / OhioLINK, 2014. http://rave.ohiolink.edu/etdc/view?acc_num=ucin1396530925.

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31

Bressert, Eli Walter. "The initial distribution of stars." Thesis, University of Exeter, 2012. http://hdl.handle.net/10036/3890.

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The primary focus of my PhD is to quantify the spatial distribution of star-forming environments from optical to radio wavelengths using data from the Hubble Space Telescope, the Very Large Telescope, the Spitzer Space Telescope, the Herschel Space Observatory, and the Caltech Submillimeter Observatory. Towards the end of my PhD study I have developed theoretical models. With these observational and theoretical avenues I have led a series of research projects to (1) quantify the initial spatial structure of pre-stellar cores and proto-stars, (2) test whether massive stars can form in isolation

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32

Kuntschner, Harald. "The star formation history of early-type galaxies in the Fornax cluster." Thesis, Durham University, 1998. http://etheses.dur.ac.uk/4849/.

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We have measured central line strengths and line-strength gradients for a complete sample of early-type galaxies in the Fornax cluster, comprising 11 elliptical and 11 lenticular galaxies, more luminous than M(_B) = -17. We find that the centres of Fornax ellipticals follow the locus of galaxies of fixed age in Worthey's models and have metallicities varying roughly from half solar to 2.5 times solar. Line-strength gradients indicate that elliptical galaxies do not show age gradients with radius but do exhibit a decrease of ~ 0.4 dex in [Fe/H] between the centre and one effective radius. The c

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Jones, Christopher William. "Dynamics, formation and segregation of the cytoplasmic chemoreceptor cluster in Rhodobacter sphaeroides." Thesis, University of Oxford, 2013. http://ora.ox.ac.uk/objects/uuid:73ce27e2-260e-4b1d-a746-cf7e7df6a02e.

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The internal organisation of bacteria is far more complex than originally thought. Many components of the cell have specific localisation patterns. Proteins are localised to many different regions of the cell by numerous mechanisms, and often their function depends on correct localisation. Bacterial and plasmid DNA are also highly organised and actively positioned. These tightly regulated positioning patterns ensure stable maintenance of genetic material. Members of the ParA/MinD family of ATPases are responsible for the segregation of a large number of bacterial chromosomes and plasmids. Rece

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Holfinger, Steven James. "PANC-1 Migration And Cluster Formation Is A Result Of Random Migration." The Ohio State University, 2011. http://rave.ohiolink.edu/etdc/view?acc_num=osu1308332896.

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35

Turner, Thomas Daniel. "Molecular self-assembly, nucleation kinetics and cluster formation associated with solution crystallisation." Thesis, University of Leeds, 2015. http://etheses.whiterose.ac.uk/11929/.

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The structural pathway from a single molecule to clustering through to nucleation during a crystallisation process is not fully understood. As such the solution state structure, nucleation kinetics and phase transformation kinetics of p-Aminobenzoic (PABA) acid are probed using a combination of in-situ crystallisation characterisation techniques and nucleation kinetic analysis methods. The solubility of alpha PABA is measured in a number of solvents where van’t Hoff analysis shows that solute-solute interactions are probable in all solvents. Solution state FTIR studies reveal the presence of a

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36

Rosander, Christian. "Characteristics of convective cloud cluster formationover Thailand through satellite image analysis." Thesis, Uppsala universitet, Luft-, vatten och landskapslära, 2007. http://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-303916.

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Weather forecasting relies on the availability of observational data as input parameters. However,such data are not readily available, because of difficulties to collect weather data due toinaccessibility to many places in the world, such as oceans or mountain regions. For this reason,satellite surveillance is a suitable tool to observe the atmosphere in regions where it is notpossible by other means. This master thesis is a study of convective cloud cluster formation over Thailand, conductedthrough satellite image analysis. Characteristics of cloud cluster formations are investigatedthrough a

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37

Simanton, Lesley Ann. "Star Cluster Populations in the Spiral Galaxy M101." University of Toledo / OhioLINK, 2015. http://rave.ohiolink.edu/etdc/view?acc_num=toledo1437587267.

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38

Emmoth, Anna. "The Legitimacy Process that Supports the Formation and Development of Cluster Initiatives : The Case of a Tourism Cluster Initiative in Dalarna." Licentiate thesis, Karlstads universitet, Centrum för tjänsteforskning, 2016. http://urn.kb.se/resolve?urn=urn:nbn:se:kau:diva-42021.

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Today, large public investments are being made with the aim of creating and developing cooperation between businesses in inter-organizational networks. Such initiatives are commonly denoted cluster initiatives and their underlying purpose are to spur innovation and regional growth. Much research has been conducted in this field, but relatively few studies have examined the process of cluster initiatives. By following the case of a regional cluster project within the tourism industry in the region of Dalarna, Sweden, the objective of this thesis is to deepen the understanding of the formation a

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Young, Teresa Marie. "Statistical thermodynamics of cluster formation in dilute colloidal and coarse-grained protein solutions." Access to citation, abstract and download form provided by ProQuest Information and Learning Company; downloadable PDF file, 206 p, 2010. http://proquest.umi.com/pqdweb?did=1997524011&sid=2&Fmt=2&clientId=8331&RQT=309&VName=PQD.

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40

Ikeda, Keisuke. "Physicochemical study on Alzheimer's amyloid-β fibril formation mediated by GM1 ganglioside cluster". 京都大学 (Kyoto University), 2009. http://hdl.handle.net/2433/124045.

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41

Bai, Lei. "The Effects of Dense Cluster Environments on Galaxies and Intracluster Dust." Diss., The University of Arizona, 2007. http://hdl.handle.net/10150/193609.

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Dense cluster environment influences the properties of galaxies and their evolution. In order to understand this environmental effect and how it evolves with time, we study the infrared (IR) properties of galaxies in three rich clusters. The IR luminosities provide us with extinction-free measurements of the star formation rates (SFRs) of these cluster galaxies. We find a strong evolution in the IR luminosity function (LF) of two z ∼ 0:8 clusters when compared to two local clusters. The evolution rate of the IR LF found in these clusters is consistent with the evolution in field IR LFs. The si

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Sheehan, Patrick D., Josh A. Eisner, Rita K. Mann, and Jonathan P. Williams. "A VLA SURVEY FOR FAINT COMPACT RADIO SOURCES IN THE ORION NEBULA CLUSTER." IOP PUBLISHING LTD, 2016. http://hdl.handle.net/10150/622165.

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We present Karl G. Jansky Very Large Array 1.3, 3.6, and 6 cm continuum maps of compact radio sources in the Orion Nebular Cluster (ONC). We mosaicked 34 arcmin(2) at 1.3 cm, 70 arcmin(2) at 3.6 cm and 109 arcmin(2) at 6 cm, containing 778 near-infrared detected young stellar objects and 190 Hubble Space Telescope-identified proplyds (with significant overlap between those characterizations). We detected radio emission from 175 compact radio sources in the ONC, including 26 sources that were detected for the first time at these wavelengths. For each detected source, we fitted a simple free-fre

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Scandariato, Gaetano. "The Initial Mass Function of the Orion Nebula Cluster from Near-Infrared Photometry." Doctoral thesis, Università di Catania, 2012. http://hdl.handle.net/10761/1027.

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The main goal of this thesis is the complete characterization of the IMF of the Orion Nebula Cluster (ONC) down to the Brown Dwarfs (BDs) regime, using ground-based Near-Infrared (NIR) photometric observations. The data taken in the framework of the Hubble Space Telescope (HST) Treasury Program on the ONC have been obtained with the wide-field imager Infrared Side Port Imager (ISPI) at the Blanco 4m telescope of CTIO, and cover an area of about 0.25 square degrees roughly centered on Theta1OriC. We observed the region in the JHKS bands with exposure times of 330 s. As a result of our survey, w

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Starostina, А. "Cluster model of territorial community development program." Thesis, Sumy State University, 2017. http://essuir.sumdu.edu.ua/handle/123456789/55778.

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The mechanism of development program formation for territorial community based on the cluster approach has been offered. The mechanism is based on a conceptual cluster model of programs. This model includes four clusters: cluster of objects that form the capability of territorial community, cluster of objects that form "overcapability" of the community; cluster of objects that define the focus area of the territorial community; and a cluster of objects that do not meet the overall focus area of local community, but generate some profit. Based on different cluster layout in program,

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Yu, Pui-ling, and 余佩玲. "Strong ram-pressure stripping and widespread star formation in the high-velocity system towards the center of the Perseus cluster." Thesis, The University of Hong Kong (Pokfulam, Hong Kong), 2015. http://hdl.handle.net/10722/211150.

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I present spectroscopic imaging of the high-velocity system (HVS) towards the central cD galaxy (NGC 1275) in the Perseus Cluster at a high spectral resolution for the first time. Previous observation suggests that the HVS is a highly inclined dusty and gas-rich galaxy moving towards the center of NGC 1275 at a high speed of 3000 km/s relative to the systemic velocity of NGC 1275 through the hot intracluster medium (ICM). If this is the case, then the HVS should be undergoing intense ram-pressure stripping. However, there is tentative evidence for ram-pressure stripping in the HVS, and further

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Pozzo, Monica. "The effect of high-mass stars on low-mass star formation." Thesis, Keele University, 2001. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.366445.

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Kriwattanawong, Wichean. "The formation and evolution of the galaxy population in the nearby cluster abell 1367." Thesis, Liverpool John Moores University, 2008. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.502762.

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48

Peralta-Quirós, Tatiana. "Exploring the relationship between destination accessibility, cluster formation and employment growth in Kendall Square." Thesis, Massachusetts Institute of Technology, 2013. http://hdl.handle.net/1721.1/82847.

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Thesis (S.M. in Transportation)--Massachusetts Institute of Technology, Department of Civil and Environmental Engineering, 2013.<br>Cataloged from PDF version of thesis.<br>Includes bibliographical references (pages 175-177).<br>The exploration of the links between transportation and land use highlights the cyclical relation of accessibility, activities and transit demand. Agglomeration theory focuses on the benefits in productivity that arise from high employment density areas when companies operate in the same sector; while cluster theory examines these centers more closely and stresses the

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Perkins, Rachel A. "Business Clustering as a Collaboration Strategy for Small Tourism Businesses Contributing to Regional Destination Branding." Thesis, Griffith University, 2021. http://hdl.handle.net/10072/407570.

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Effective branding for destinations encourages visitation and ensures the financial stability of regions that rely on tourist expenditure. Literature reveals however, that the destination branding process is not straightforward, particularly in regional destinations of which Australia’s tourism industry is largely comprised. Scholars advocate for collaboration as a solution to enacting destination branding, but, the feasibility and practicality of working together presents many challenges. It is therefore crucial that collaboration is further understood by honing in on the collaborative strate

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Barlović, Robert. "Traffic jams cluster formation in low-dimensional cellular automata models for highway and city traffic /." [S.l. : s.n.], 2003. http://deposit.ddb.de/cgi-bin/dokserv?idn=969248830.

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