It is known that active galaxies have small core regions because we can see them in images! These small regions known as uassars emit perful amounts of both radio waves and gamma rays...
Metal-core is more popular because is easier to listen.
In the core of an apple there are apple seeds (pips); In the core of the Earth there is a ball of Iron; In the core of the Sun there is a fusing ball of hydrogen plasma, while core memory of a computer contains circular ferro magnets threaded onto a lattice or mesh of wires.
Seeing as Core 2 Duo sounds redundant (since 2 is the same as duo), I would say that Duel Core is more accurate, unless they are two different things. If they aren't the same, core 2 Duo could be an upgrade from duel core, but that just might be just me.
i believe the heater core is leaking, a small pin hole leak can generate a lot of smell.
It would be best to disconnect the coolant lines and flush the core after the radiator flush. This will clear any sediment from the core.
Consider the giant elliptical galaxy M87, it has a very small, bright nucleus and a visible jet of matter 1800 PC long racing out of its core. Radio observations show that the nucleus must be no mre than a light week in diameter.
All galaxies have a dense core of stars. Spiral galaxies, however, have arms that are often visible. There are two kinds of spiral galaxies: barred, where there appears to be a line running from arm to arm through the core, and ordinary, where there is no bar.
A Seyfert galaxy is a spiral galaxy with an active core.
Economists have identified regions of the world called core regions of economic development. The core regions are North America, Europe and Japan. China is not currently listed because it does not have the model as described below: The core regions have these characteristics; they have economic diversification; * The nations have a high standard of living; * They are leaders in technology;and * Productivity levels are high.
As our telescopes improve, we have discovered that there are supermassive black holes in the cores of many, perhaps most galaxies. Scientists have long known that the galaxies did not appear to have enough mass to stay together; since they DO stay together, there has to be mass - a LOT of mass - that we aren't seeing. Since we don't know anything other as a core for a galaxy then, the Core itself must be called "The Black Hole".
Core-periphery structures can promote economic growth and specialization, leading to higher productivity in core regions and increased access to markets for peripheral regions. They can also facilitate the flow of knowledge, technology, and skills between regions, supporting overall development. However, there are risks of unequal development, with core regions often benefiting more than peripheral regions in terms of resources and opportunities.
Active political participation by all citizens is the core of which political system
The central core has 5 regions which helps to regulate the basic life processes.
There are generally three types of galaxies: spiral galaxies, elliptical galaxies, and irregular galaxies. Spiral galaxies like the Milky Way have a disk shape with arms of stars spiraling out from a central core. Elliptical galaxies are shaped like ellipses and contain mostly older stars. Irregular galaxies have a less defined shape and tend to have a mix of young and old stars.
Outer core From 4400'C in the outer regions near the mantle, to around 6100'C in the inner regions near the inner core (7,952 to 11,000oF).Inner core--between 5,000 and 7,000 degrees C (9,000 to 12,630oF).
Core-periphery refers to a geographic concept where a core region is economically and politically dominant, while the periphery regions are less developed or dependent on the core. This concept implies a hierarchical relationship between different regions based on levels of economic development and power.
All types of galaxies have a core with a high star density. All galaxies with "arms" are called Spiral Galaxies, of which there are sub-types related to the shape of the arms.