3,340 research outputs found
Report of Resolutions Committee
Note: The report of the Committee has been reduced to publish here the actual resolutions prepared, recommended, and adopte
A comparative study of CO adsorption on flat, stepped and kinked Au surfaces using density functional theory
Our ab initio calculations of CO adsorption energies on low miller index
(111), (100), stepped (211), and kinked (532) gold surfaces show a strong
dependence on local coordination with a reduction in Au atom coordination
leading to higher binding energies. We find trends in adsorption energies to be
similar to those reported in experiments and calculations for other metal
surfaces. The (532) surface provides insights into these trends because of the
availability of a large number of kink sites which naturally have the lowest
coordination (6). We also find that, for all surfaces, an increase in CO
coverage triggers a decrease in the adsorption energy. Changes in the
work-function upon CO adsorption, as well as the frequencies of the CO
vibrational modes are calculated, and their coverage dependence is reported.Comment: 18 pages, 4 figure
Missouri libraries, 1915-1935
Handbook authorized by the Executive board of the Missouri Library Association--Introduction
Annual Meeting; Resolutions; Report of Committee on Uniform System of Numbers for Code of the State of Washington; Report of Committee on Selection of Judges; Report of State Bar Delegate to American Bar Association Meeting
Sound and light in periodically microstructured materials
EThOS - Electronic Theses Online ServiceGBUnited Kingdo
Observations of Binary Stars with the Differential Speckle Survey Instrument. V. Toward an Empirical Metal-Poor Mass-Luminosity Relation
In an effort to better understand the details of the stellar structure and
evolution of metal poor stars, the Gemini North telescope was used on two
occasions to take speckle imaging data of a sample of known spectroscopic
binary stars and other nearby stars in order to search for and resolve close
companions. The observations were obtained using the Differential Speckle
Survey Instrument, which takes data in two filters simultaneously. The results
presented here are of 90 observations of 23 systems in which one or more
companions was detected, and 6 stars where no companion was detected to the
limit of the camera capabilities at Gemini. In the case of the binary and
multiple stars, these results are then further analyzed to make first orbit
determinations in five cases, and orbit refinements in four other cases. Mass
information is derived, and since the systems span a range in metallicity, a
study is presented that compares our results with the expected trend in total
mass as derived from the most recent Yale isochrones as a function of metal
abundance. These data suggest that metal-poor main-sequence stars are less
massive at a given color than their solar-metallicity analogues in a manner
consistent with that predicted from the theory
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