Looking past inessential complexities to explain the Internet's simple yet daring design.
Crystalline silicon transistors offer better performance and higher speeds than amorphous or poly-silicon transistors. This leads to higher resolution, larger displays, and better performance of the AMLCD. Using pre-fabricated crystalline silicon devices allows for the advantage of more complex circuit design within the pixel such as the incorporation of storage capacitors, or multi-device circuits at each pixel. This technique also offers a simplified, lower cost alternative to present production processes.
Abstract The new silyl derivatives (Ia)‐(Id) are prepared by reaction of the trisilylsilyl‐Li compound (III) with the appropriate metal halides (IIa)‐(IId).
NGC 3079 is a remarkable spiral galaxy which exhibits an unusual range of nuclear activity. Viewed edge-on, it harbors a reddened LINER (Low Ionization Nuclear Emission-line Region) that is kinematically complex, with several distinct components of Ha emission. It also contains a compact, flat spectrum nuclear radio source, and shows well-defined, kiloparsec-scale radio lobes of considerable complexity, as well as a smaller loop of Hα+[N II] emission extending approximately along the minor axis of the galaxy. The optical emission lines indicate that gas is outflowing from the nucleus in an energetic, bipolar outflow or “galactic superwind.” Armus et al. (1990) have suggested that this wind is driven by a powerful, central starburst. A number of different lines of evidence — its infrared brightness (measured by IRAS, the extended 10 μm emission, the spatially coincident, circumnuclear molecular gas, and the extremely luminous H2O maser — point to the presence of ongoing, vigorous star formation within the nucleus, in agreement with this idea. However, other authors (e.g., Irwin and Sofue 1992; Filippenko and Sargent 1992) argue that the nuclear activity originates from an AGN, perhaps supplemented by a powerful starburst.