This study aims to determine the impact of using social media on knowledge sharing for high school teachers in Bima Regency, with capital represented by variables, namely network ties, shared vision and trust as mediating variables. To test hypothesis, researcher used data collected through questionnaires a total 237 respondents purposive convenience techniques sampling statistical analysis, St...

Not much effort has been made to explore Bima as a historical node within the framework of Islamic epistemology in Nusantara. In fact, area that was formerly known Kingdom became one important trading ports connected spice shipping routes east Because its strategic location and significance connection point Nusantara, end can not only be read an economic reality, but also cultural reality which...

Uranium nitride complexes are attractive targets for chemists as molecular models the bonding, reactivity, and magnetic properties of next-generation nuclear fuels, but these molecules uncommon can be difficult to isolate due their high reactivity. Here, we describe synthesis three new multinuclear uranium complexes, [U(BCMA)2]2(μ-N)(μ-κ1:κ1-BCMA) (7), [(U(BIMA)2)2(μ-N)(μ-NiPr)(K2(μ-η3:η3-CH2CH...

Mate pair library sequencing is an effective and economical method for detecting genomic structural variants and chromosomal abnormalities. Unfortunately, the mapping and alignment of mate-pair read pairs to a reference genome is a challenging and time-consuming process for most next-generation sequencing alignment programs. Large insert sizes, introduction of library preparation protocol artif...

The power output in luminous infrared galaxies (LIGs, LIR,(,1011L 8 , Hi, == 75 km s-l Mpc1) can approach the bolometric luminosity of quasars and can be provided by either starbursts or dust-enshouded QSOs, or both. Most LIGs appear to comprise of mergers of gas-rich galaxies. So, intense bursts of star formation apparently result from interaction and merging of galaxies, but the exact physica...

We discuss BIMA (Berkeley Illinois Maryland Association) data and present new high quality optical and near-IR Keck images of the bright radio ring PKS 1830–211. Applying a powerful new deconvolution algorithm we have been able to identify both images of the radio source. In addition we recover an extended source in the optical, consistent with the expected location of the lensing galaxy. The s...