TY - GEN A1 - Sandin, Christer A1 - Steffen, Matthias A1 - Jacob, Ralf A1 - Schönberner, Detlef A1 - Rühling, Ute A1 - Hamann, Wolf-Rainer A1 - Todt, Helge Tobias T1 - The role of heat conduction to the formation of [WC]-type planetary nebulae T2 - Proceedings of the International Astronomical Union N2 - X-ray observations of young Planetary Nebulæ (PNe) have revealed diffuse emission in extended regions around both H-rich and H-deficient central stars. In order to also repro-duce physical properties of H-deficient objects, we have, at first, extended our time-dependent radiation-hydrodynamic models with heat conduction for such conditions. Here we present some of the important physical concepts, which determine how and when a hot wind-blown bubble forms. In this study we have had to consider the, largely unknown, evolution of the CSPN, the slow (AGB) wind, the fast hot-CSPN wind, and the chemical composition. The main conclusion of our work is that heat conduction is needed to explain X-ray properties of wind-blown bubbles also in H-deficient objects. T3 - Zweitveröffentlichungen der Universität Potsdam : Mathematisch-Naturwissenschaftliche Reihe - 582 KW - conduction KW - hydrodynamics KW - planetary nebulae: general Y1 - 2019 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-413702 SN - 1866-8372 IS - 582 SP - 494 EP - 495 ER - TY - JOUR A1 - Sandin, C. A1 - Steffen, M. A1 - Schoenberner, D. A1 - Rühling, Ute T1 - Hot bubbles of planetary nebulae with hydrogen-deficient winds I. Heat conduction in a chemically stratified plasma JF - Frontiers in psychology N2 - Heat conduction has been found a plausible solution to explain discrepancies between expected and measured temperatures in hot bubbles of planetary nebulae (PNe). While the heat conduction process depends on the chemical composition, to date it has been exclusively studied for pure hydrogen plasmas in PNe. A smaller population of PNe show hydrogen-deficient and helium-and carbon-enriched surfaces surrounded by bubbles of the same composition; considerable differences are expected in physical properties of these objects in comparison to the pure hydrogen case. The aim of this study is to explore how a chemistry-dependent formulation of the heat conduction affects physical properties and how it affects the X-ray emission from PN bubbles of hydrogen-deficient stars. We extend the description of heat conduction in our radiation hydrodynamics code to work with any chemical composition. We then compare the bubble-formation process with a representative PN model using both the new and the old descriptions. We also compare differences in the resulting X-ray temperature and luminosity observables of the two descriptions. The improved equations show that the heat conduction in our representative model of a hydrogen-deficient PN is nearly as efficient with the chemistry-dependent description; a lower value on the diffusion coefficient is compensated by a slightly steeper temperature gradient. The bubble becomes somewhat hotter with the improved equations, but differences are otherwise minute. The observable properties of the bubble in terms of the X-ray temperature and luminosity are seemingly unaffected. KW - conduction KW - hydrodynamics KW - planetary nebulae: general KW - stars: AGB and post-AGB KW - stars: Wolf-Rayet KW - X-rays: stars Y1 - 2016 U6 - https://doi.org/10.1051/0004-6361/201527357 SN - 1432-0746 VL - 586 PB - EDP Sciences CY - Les Ulis ER - TY - JOUR A1 - Distelmeyer, Jan T1 - From object to process BT - Interface politics of networked computerization JF - Artnodes N2 - One of the most difficult tasks today is trying to grasp the presence of computing. The almost ubiquitous and diverse forms of networked computers (in all their stationary, mobile, embedded, and autonomous modes) create a nearly overwhelming complexity. To speak of what is here evading and present at the same time, the paper proposes to reconsider the concept of interface, its historical roots, and its heuristic advantages for an analysis and critique of the current and especially everyday spread of computerization. The question of interfaces leads to isolable conditions and processes of conduction, as well as to the complexity of the cooperation formed by them. It opens both an investigative horizon and a mode of analysis, which always asks for further interface levels involved in the phenomenon I am currently investigating. As an example, the paper turns to the displacement of the file with the launch of the iPhone in 2007 and its comeback in 2017 with the "Files" apps. Both developments are profoundly related to the establishment of computers as permanently networked machines, whereby their functionality, depresentations, and ideology come into focus. KW - interface KW - conduction KW - network KW - ideology KW - depresentation KW - digital objects Y1 - 2019 U6 - https://doi.org/10.7238/a.v0i24.3300 SN - 1695-5951 IS - 24 SP - 83 EP - 90 PB - Universitat Oberta de Catalunya CY - Barcelona ER -