since the time of western modernity, knowledge is compartmentalized into differentiated fields. this has however not mitigated the influence of natural science model of theorizing on social sciences. as a result, the discipline of organization theory has grown without the influence of abstract, ephemeral and metaphysical fields such as religion, history, mystic philosophy, arts and literature. ...

We report Sr, Pd and Ag abundances for a sample of metal-poor field giants and analyze a larger sample of Y, Zr, and Ba abundances. The [Y/Zr] and [Pd/Ag] abundance ratios are similar to those measured for the r-process-rich stars CS 22892-052 and CS 31082-001. The [Pd/Ag] ratio is larger than predicted from the solar-system r-process abundances. The constant [Y/Zr] and [Sr/Y] values in the fie...

New axisymmetric (2D) models for dust-driven winds of C-stars are presented which include hydrodynamics with radiation pressure on dust, equilibrium chemistry and time-dependent dust formation with coupled grey Monte Carlo radiative transfer. Considering the most simple case without stellar pulsation (hydrostatic inner boundary condition) these models reveal a more complex picture of the dust f...

The theory of symbolic racism places its origins in a blend of anti-Black affect and conservative values, particularly individualism. We clarify that hypothesis, test it directly, and report several findings consistent with it. Study 1 shows that racial prejudice and general political conservatism fall into 2 separate factors, with symbolic racism loading about equally on both. Study 2 found th...

Where do stars come from? Human beings have thought about this question for thousands of years and have proposed many different explanations, but scientists have only had the technology to observe the places where stars are forming for a few decades. This is because stars form inside cold “dusty” clouds in space that are invisible to our eyes and invisible to telescopes that study visible light...

We determine the parallax and proper motion of the flaring, non-thermal radio star GMR A, a member of the Orion Nebula Cluster, using Very Long Baseline Array observations. Based on the parallax, we measure a distance of 389 −21 parsecs to the source. Our measurement places the Orion Nebula Cluster considerably closer than the canonical distance of 480 ± 80 parsecs determined by Genzel et al. (...