斑驳 发表于 2025-3-23 09:57:32
http://reply.papertrans.cn/89/8814/881348/881348_11.pngResign 发表于 2025-3-23 17:06:11
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.Desert 发表于 2025-3-23 21:48:26
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.receptors 发表于 2025-3-24 00:33:54
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.certain 发表于 2025-3-24 03:21:17
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 collapsatopic 发表于 2025-3-24 06:31:08
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歌剧等 发表于 2025-3-24 10:49:59
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.Defense 发表于 2025-3-24 16:32:20
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http://reply.papertrans.cn/89/8814/881348/881348_19.pngDiuretic 发表于 2025-3-25 02:32:38
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