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C#從入門到精通（微視頻精編版）（共2冊）

為了解決m/s km/h換算的問題，作者明日科技 這樣論述：

本書淺顯易懂，實例豐富，詳細介紹了C#開發需要掌握的各類實戰知識。 　　 全書分為兩冊：核心技術分冊和強化訓練分冊。核心技術分冊共20章，包括搭建C#開發環境、初識C#程式結構、C#語言基礎、運運算元、條件控制語句、迴圈控制語句、陣列的使用、字串處理、類和物件、繼承和多態、程式調試與異常處理、Windows表單程式設計、Windows控制項的使用、C#操作資料庫、Entity Framework程式設計、檔及資料流程技術、GDI+繪圖應用、Socket網路程式設計、多執行緒程式設計技術和庫存管理系統等內容。通過學習，讀者可快速開發出一些中小型應用程式。強化訓練分冊共17章，

通過大量源於實際生活的趣味案例，強化上機實踐，拓展和提升C#開發中對實際問題的分析與解決能力。

Galaxies in the Local Volume

為了解決m/s km/h換算的問題，作者Koribalski, B. s. (EDT)/ Jerjen, H. (EDT) 這樣論述：

The Local Volume' (ie, the sphere of radius 10 Mpc centered on the Local Group) is known to contain at least 500 known galaxies, many of which congregate in well-known groups like the Local Group, the relatively loose Sculptor Group, and the more compact Centaurus A group. Accurate distances are no

w available for the majority of these nearby galaxies, allowing us to visualise the Local Volume in 3D, study the local Hubble flow and its dispersion, the (baryonic) Tully-Fisher relation, the local star formation density, etc. Individual galaxies in the Local Volume can be studied in amazing detai

l across a large range of wavelengths (some stunning examples are compiled in the Multiwavelength Astronomy pages).The first catalog of galaxies within 10 Mpc was compiled by Kraan-Korteweg & Tammann (1979); it contained 179 galaxies. Following numerous updates, the latest Catalog of Neighboring Ga

laxies' was presented by Karachentsev et al. (2004); it contains 451 galaxies. They find that about 85% of the LV population are dwarf galaxies which contribute approx. 4% to the local optical luminosity density and roughly 10-15% to the local HI mass density. For the majority of galaxies within 8 M

pc we currently have quite reliable, independent distance estimates either from the luminosity of Cepheids, the tip of the red giant branch (TRGB), or surface brightness fluctuations (SBF).Several large surveys of nearby galaxies have recently been carried out or are in progress. E.g., The Westerbo

rk observations of neutral Hydrogen in Irregular and SPiral galaxies' (WHISP, Swaters et al. 2002), which is based on the Uppsala General Catalogue of Galaxies (UGC; Nielson 1973), provides HI distributions and velocity fields of about 200 gas-rich galaxies with declinations larger than +20 degrees

and velocities less than 2000 km/s. This is complemented by The Ha Galaxy Survey' (HaGS; James et al. 2004), also based on the UGC, which provides star formation parameters for a large number of mostly northern galaxies. The HI Nearby Galaxy Survey' (THINGS; Walter, Brinks, de Blok et al. 2004), w

hich provides high-resolution HI imaging of initially 36 galaxies with declinations larger than -30 degrees, has just been completed at the Very Large Array (VLA). The THINGS sample is targeting galaxies from The Spitzer Nearby Galaxies Survey' (SINGS, Kennicutt et al. 2003), a comprehensive infrar

ed imaging and spectroscopic survey of 75 nearby galaxies with distances less than 30 Mpc, as well as key objects from the Spitzer GTO list. SINGS is supplemented by high-resolution studies at many other wavelengths covering the entire spectrum from X-ray to radio. Another multi-wavelength study is

The Survey for Ionization in Neutral Gas Galaxies' (SINGG, Meurer et al. 2006, Hanish et al. 2006), the largest star formation survey of an HI-selected sample (based on The HI Parkes All-Sky Survey', HIPASS) and its sister surveys SUNGG and SONGG, based on GALEX ultraviolet and Spitzer infrared ob

servations, respectively. Surveys of nearby galaxies currently underway in Australia include The Galactic All Sky Survey' (GASS), obtained with the Parkes 64-m telescope, The Local Volume HI Survey' (LVHIS), obtained with the Australia Telescope Compact Array (ATCA), and the Local Sphere of Influ

ence H-band survey' (LSI), obtained with the Anglo-Australian Telescope (AAT).Given the many recent advances in our understanding of the star formation and ISM composition of nearby galaxies and more generally in the field of Near-Field Cosmology', which are mostly based on the large amounts and su

perb quality of new ground- and space-based multi-wavelength data, it is timely to hold a conference on the subject and review the Local Volume by combining observations, simulations and theoretical developments. We hope to provide a vibrant forum for presentations and discussions accross a broad ra

nge of astrophysical topics, including what may be possible with future facilities such as the Atacama Large Millimeter Array (ALMA), and the international Square Kilometre Array (SKA). B.S. Koribalski (Physics Diploma and PhD from the University of Bonn, Germany; now Senior Research Scientist at

the CSIRO Australia Telescope National Facility; PI of the ＂Local Volume HI Survey＂ (LVHIS), etc.)

組織同形化與動態能力對電商營運模式之探討 ：以外貿廠商為例

為了解決m/s km/h換算的問題，作者黃偉誠 這樣論述：

近年來行動科技的普及，使電子商務不但改變了消費方式，更帶動全球B2B和B2C電商市場規模急速成長，甚至改變全球交易行為和商業模式，更因為新冠疫情肆虐催化下，以致加速全球電子商務發展的腳步和節奏，使各電子商務平台迅速成長崛起，消費者需求越來越難以捉摸，使同業間的競爭越來越激烈，加上因為賣家數量的增加，使電商市場呈現出同質化現象越來越嚴重，投入跨境電商之企業趨同形現象發展，其中同形化範疇含括了物流、品牌行銷、廣告、數據分析、通路、零售及店舖經營、媒體、創意、人才培養等多方面，同形化市場加速了廠商間競爭窘境。有鑑於此，本研究欲探討外貿廠商投入電商營運活動中，在網路行銷、關鍵字規劃與分析、數據分析、

文案與數位媒體行銷等方式趨向模仿同形時，如何在同形化的電商市場中審視自身資源，充分發揮企業動態能力，打造自身差異化，進而擬訂營運模式。本研究採個案訪談法，共訪談五家曾獲得電子商務成就或優異表現之個案公司，探討個案廠商投入電商營運之動機，並如何從市場同形化過程中找出企業營運模式和發展動態能力以增加企業生存機會。本研究結果發現，在組織同形的跨境電商市場中，個案企業在投入跨境電商皆會使用投放廣告、官網SEO、Google關鍵字、Google ads、影音行銷商品影片在間接與平台一同串連，來達到曝光度最大化；平台選擇上，發現皆以阿里巴巴國際站為主要使用的跨境電商平台，因為阿里巴巴國際站長年開設客製化的

企業培訓課程輔助台灣中小企業邁入外貿，上述皆是在高度競爭同形化的電商市場中必須做的事情；最後真正突破同形化的關鍵為企業不斷增進自身企業能力以及審視整體市場來調整自身策略，進而從同形化中異形出自身公司的電商DNA，顯示出其企業自身差異化，達到企業的永續經營，在跨境電商市場之競爭趨向同形的現象中真正脫穎而出關鍵。本研究期能透過此研究，讓中小企業了解跨境電商之營運模式，讓有意轉型之中小企業了解企業在同形化市場當中具備之電商思維態度與能力，且需能與時俱進的調整營運方式，以追求企業成長和發展。