Potential of colors for determining age and metallicity of stellar populations

Colors are usually not used for constraining stellar populations because they are thought to have the well-known agemetallicity degeneracy, but some recent works show that colors can also be used. A simple stellar population synthesis model is widely used, but there is no analysis for its colors. We try to find colors that can potentially be used to determine the age and metallicity of stellar populations by the standard model. Principal component analysis and relative sensitive parameter techniques are used in this work. As a result, U-K, U-H, U-J, B-K, B-H, U-I, B-J, and V-K are found to be more important for studying populations than others. Pairs of colors such as B-K and B-V are found to be able to disentangle the stellar age-metallicity degeneracy via the high-resolution model, while pairs such as U-K and R-I may be used instead when the low-resolution model is used. Furthermore, the u-g and r-i colors of the low-resolution model seem to have the same potential, but there are no such colors for the high-resolution one. In conclusion, some colors have been shown to have the potential to determine the age and metallicity of stellar populations, but relative metallicity and age sensitivities of colors in different stellar population synthesis models are usually different. In addition, minor star formations will make star systems look younger and more metal rich than their dominating populations.Comment: Accepted for publication in A&A, 6 pages, 7 figure

CFD investigation of blind-tee effects on flow mixing mechanism in subsea pipelines

Blind tees are widely used in subsea pipelines to enhance the mixing conditions of oil and gas products, but their structural design still relies on experience. In this paper, a series of numerical investigations have been carried out on blind-tee pipes in order to develop an in-depth understanding of their mixing mechanism and clarify the effects of blind-tee structures on the pipe flow. Firstly, the three-dimensional flow conditions in a typical blind tee have been simulated under different Reynolds numbers to investigate the mixing mechanism. Two critical Reynolds numbers for the vortex generations in blind tees are determined in the laminar flow regime, and the fitting curves of blind-tee vorticity dissipations are obtained. Then, the geometrical parameters, including the radial size ϕ, axial length (BSL) and position of the blind section, are varied systematically to study their effects on the flow characteristics and mixing conditions. The results indicate that increasing ϕ and BSL in an appropriate range can strengthen the flow circulation and promote the fluid exchange. Finally, an optimal configuration is obtained, which can improve the mixing capacity of blind tee by 53% in terms of the volume average vorticity as compared to the typical structure.publishedVersio