Titlebook: Submillimetre Studies of Prestellar and Starless Cores in the Ophiuchus, Taurus and Cepheus Molecula; Katherine Miranda Pattle Book 2017 S

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The Taurus Molecular Cloud,This chapter discusses the Taurus molecular cloud. Sources are extracted from the SCUBA-2 850-.m data, Herschel 250-.m data, and Herschel 250-.m data filtered to match the spatial scales detectable with SCUBA-2.

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The Cepheus Flare,This chapter discusses the Cepheus Flare molecular clouds. Sources are extracted from the SCUBA-2 850-.m data and characterised using flux densities measured from the 850-.m data and temperatures provided by the Herschel Gould Belt Survey.

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Discussion,This chapter compares the Ophiuchus, Taurus and Cepheus Flare regions. An evolutionary model for initially pressure-confined starless cores is proposed and discussed. A modified and expanded version of the second half of this chapter has been published by Pattle (2016), Monthly Notices of the Royal Astronomical Society, vol. 459, p. 4255.

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Katherine Miranda PattleNominated as an outstanding PhD thesis by the University of Central Lancashire, Preston, United Kingdom.Demonstrates new methods for virial analysis in order to determine the stability against collaps

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2190-5053 ess core may evolve due to virial stability rather than gravitational collapse, which means that a core can only be definitively considered to be prestellar if it is gravitationally bound.978-3-319-85935-4978-3-319-56520-0Series ISSN 2190-5053 Series E-ISSN 2190-5061

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Book 2017tion of starless cores in the “virial plane”, demonstrating that a pressure-confined starless core may evolve due to virial stability rather than gravitational collapse, which means that a core can only be definitively considered to be prestellar if it is gravitationally bound.

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e TSV power consumption effectively. In this chapter, a coding technique is presented that aims for an increase in the performance of TSVs and metal wires. The method takes the edge effects into account, which enables a much higher improvement in the TSV performance than previous techniques and, for