A Component Framework for Java-based Real-time Embedded Systems

Rank (CORE): A.International audienceThe Real-Time Specification for Java (RTSJ) is becoming a popular choice in the world of real-time and embedded programming. However, RTSJ introduces many non-intuitive rules and restrictions which prevent its wide adoption. Moreover, current state-of-the-art frameworks usually fail to alleviate the development process into higher layers of the software development life-cycle. In this paper we extend our philosophy that RTSJ concepts need to be considered at early stages of software development, postulated in our prior work, in a framework that provides continuum between the design and implementation process. A component model designed specially for RTSJ serves here as a cornerstone. As the first contribution of this work, we propose a development process where RTSJ concepts are manipulated independently from functional aspects. Second, we mitigate complexities of RTSJ-development by automatically generating execution infrastructure where real-time concerns are transparently managed. We thus allow developers to create systems for variously constrained real-time and embedded environments. Performed benchmarks show that the overhead of the framework is minimal in comparison to manually written object-oriented approach, while providing more extensive functionality. Finally, the framework is designed with the stress on dynamic adaptability of target systems, a property we envisage as a fundamental in an upcoming era of massively developed real-time systems

The relation between accretion rate and jet power in early-type galaxies with thermally unstable hot atmospheres

High Energy AstrophysicsGalaxie

The relation between accretion rate and jet power in early-type galaxies with thermally unstable hot atmospheres

We use Chandra X-ray data and Very Large Array radio observations for a sample of 20 nearby, massive, X-ray bright, early-type galaxies to investigate the relation between the Bondi accretion rates and the mechanical jet powers. We find a strong correlation ($\rho = 0.96$; BF$_{10} > 100$) between the Bondi accretion power, $P_{\text{Bondi}}$, and mechanical jet power, $P_{\text{jet}}$, for a subsample of 14 galaxies, which also host cool H$\alpha$+[NII] line emitting gas and thus likely have thermally unstable atmospheres. The results indicate that in all galaxies with thermally unstable atmospheres the cooling atmospheric gas feeds the central black holes at a similar jet-to-Bondi power ratio. For five out of six galaxies with no signs of H$\alpha$+[NII] emission, however, the behaviour is different and the jet-to-Bondi power ratio is lower by 1-2 orders of magnitude. We also investigate the dependence of jet power on individual quantities in the Bondi formula such as the supermassive black hole mass ($M_{\bullet}$) and the specific entropy of the gas ($K$) at the Bondi radius. For the subsample of H$\alpha$+[NII] emitting galaxies, we find a very tight correlation of $P_{\text{jet}}$ with $M_{\bullet}$ ($\rho = 0.92$; BF$_{10} > 100$) and, although poorly constrained, a hint of an anti-correlation for $P_{\text{jet}}$ and $K$ ($\rho = -0.46$; BF$_{10} = 1.2$).Comment: 29 pages, 12 figure