Hnr Indstu In BCT

This is a stand-alone independent study designed by the student and faculty sponsor that involves frequent interaction between instructor and student. Qualitative and quantitative enrichment must be evident on the proposed contract before consent is given to undertake the study.

Communicating Sustainability

Effective communication is not always easy or natural, but it can be learned. This course provides a platform to learn and practice principles of professional communication (through presentations, writing, and audio/visual media) in the field of construction and sustainable building. Through various class exercises and assignments, students attain the skills that are required to succinctly get a message across and connect with an audience.

Construction Materials&Methods

Provides an introductory overview of the main materials used in commercial construction: steel, concrete, and masonry (wood is covered in BCT 304 / ECO 624). After receiving an introduction into fundamental principles of structural, physical and long-term performance, students learn about material and product manufacturing techniques and how they relate to mechanical and non-mechanical properties of the various materials. Common construction methods are introduced and building details are explored.

Hnr Indstu In BCT

This is a stand-alone independent study designed by the student and faculty sponsor that involves frequent interaction between instructor and student. Qualitative and quantitative enrichment must be evident on the proposed contract before consent is given to undertake the study.

Advanced Topic

Topics of special interest not covered in regular courses at the present time. Recent examples include material in infrared astronomical techniques and instrumentation; high resolution astronomy, including interferometry and speckle methods; and the use of modern computer hardware and software in astronomical problems involving large data sets.

Interstellar Medium

Describes the gas and dust components of the interstellar medium in ionized regions, atomic clouds, and molecular clouds. Shows how data from optical, infrared, and radio wavelengths can be utilized to determine density, temperature, composition, and dynamics of the various phases of the ISM. Comparison of these results with theoretical models. Includes an overview of the processes that affect the evolution of the ISM including the incorporation of gas and dust into stars, the effect of HII regions and young stellar objects, and the return of matter from evolved stars and supernovae.
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