UGO described Lucario as "a new breed of Pokémon, with a cooler, more dangerous look. It's quick and possesses a damaging set of attacks", yet called it lame due to its status as a Pokémon. IGN called its presence in "Super Smash Bros. Brawl" "a bit on the head scratching side" in light of more familiar characters in the title such as Pikachu. Although another editor stated that it would make sense for "Pokémon" to be represented by a fighting-type Pokémon, since "Super Smash Bros Brawl" is a fighting game. GamesRadar described it as an "all-around bad-ass" and "the Bruce Lee of Pokémon", suggesting its design as similar to the Egyptian God Anubis. Beckett "Pokémon" Unofficial Collector editor Sean Cooper stated that Lucario had grown popular in recent years due to his starring role in "Lucario and the Mystery of Mew" and his appearance in "Super Smash Bros. Brawl".
Cacabelos
Cacabelos, is a municipality in the province of León, Castilla y León, Spain. According to the 2008 census (INE), Cacabelos had 5,477 people.
Cacabelos is well known for its wines.
Cabrillanes
Cabrillanes is a municipality in the province of León, Castile and León, Spain. In 2010, (INE), 964 people lived there people.
Camponaraya
Camponaraya is a municipality in the province of León, Castile and León, Spain. According to the 2004 census (INE), 3,411 people lived there.
Villamañán
Villamañán is a town in the southwest of the province of León, Spain. It is in the area known as "Esla", in the autonomous community of Castile and León.
It was originally known as Villamagna, but the name evolved to its current version, Villamañán.
La Bañeza
La Bañeza is a municipality in the province of León, Castile and León, Spain. According to the 2005 census (INE), 10,123 people lived there.
Cármenes
Cármenes is a municipality in the province of León, Castile and León, Spain. According to the 2004 census (INE), 425 people lived there.
Villablino
Villablino ("Vitsablinu", in Leonese language) is a municipality in the province of León, Castile and León, Spain. According to the 2004 census (INE), the municipality has 12,212 people.
Castrotierra de Valmadrigal
Castrotierra de Valmadrigal is a municipality in the province of León, Castile and León, Spain. According to the 2004 census (INE), it had 142 people.
El Burgo Ranero
El Burgo Ranero is a municipality in the province of León, Castile and León, Spain. According to the 2004 census (INE), the municipality has a population of 894 inhabitants.
Villamanín
Villamanín is a municipality in the province of León, Castile and León, Spain. According to the 2004 census (INE), the municipality has 1,161 people.
Carucedo
Carucedo is a municipality in the province of León, Castile and León, Spain. According to the 2010 census (INE), 642 people lived there.
Luyego
Luyego is a municipality in the province of León, Castile and León, Spain. According to the 2004 census (INE), the municipality has 887 people.
Destriana
Destriana is a municipality in the province of León, Castile and León, Spain. According to the 2004 census (INE), 736 people lived there.
Igüeña
Igüeña is a municipality in the province of León, Castile and León, Spain. According to the 2004 census (INE), 1,702 people lived there.
Hertzsprung–Russell diagram
The Hertzsprung-Russell diagram is a graph of many stars. It shows the relation between stars' luminosity (that is, how bright they are) and their temperature (how hot they are). These diagrams are not pictures or maps of the locations of the stars. Rather, Hertzsprung-Russell diagrams plot each star on a graph measuring the star's brightness versus its temperature. Hertzsprung-Russell diagrams are also called H-R diagrams or HRDs.
You can see an example of a Hertzsprung-Russell diagram to the right. This diagram is based on measurements from 23,000 stars in our Milky Way galaxy. The Hertzsprung-Russell diagram is named after its creators, astronomers Ejnar Hertzsprung and Henry Norris Russell.
The vertical axis of a Hertzsprung-Russell diagram shows the luminosity or brightness of the stars, as if they were all measured from the same distance. Another term for this is absolute magnitude. The brighter a star is, the higher its plot will be on this chart.
The horizontal axis shows the surface temperature of the stars. However, the temperatures go "down", not up, as you move to the right. That is, the left of the diagram contains stars with the highest temperature plots (greater than 30,000 Kelvins) while the right shows stars with temperatures of only 3000K.
In general, the temperature of a star relates to its color. At the top of the chart, along with the temperatures, are the Spectral Classes. The hottest stars are blue-white (class O), those in the middle temperatures are yellow (class G) and the coolest ones are red (class M). (Of course, when we say "coolest" about stars, we must realize that the lowest temperature for a star is almost 5000 degrees Fahrenheit.)
As a matter of fact, when Hertzsprung-Russell diagrams were developed in the early 1900's, astronomers did not know how to find out the temperature of a star. The first diagrams plotted stars' absolute magnitude (where "adding" one meant the brightness would go "down" by about two and a half times) against color, represented by the spectral classes from blue-white to red.
As you can see, stars tend to fall only into certain regions of the diagram when graphed in this way. All stars in a given area of a Hertzsprung-Russell diagram share similar luminosities and temperatures. The main region where stars appear is the diagonal curved line, going from the upper-left (hot and bright) to the lower-right (cooler and less bright). This is called the Main Sequence. Above the main sequence is another region containing the red giants. Below is a curved line representing the white dwarfs.
These collections of stars by brightness and temperature are important when talking about stellar evolution. In general, stars are created in the main sequence. (Of course, when we say ""in" the main sequence" we really mean "having a brightness and a temperature that causes them to be plotted within the main sequence on a Hertzsprung-Russell diagram.") After billions of years, they expand into red giants. Then, after another one or two billion years, they shrink into white dwarfs.
It was only in the 1930's and 1940's that scientists began to understand the role of nuclear fusion in creating and keeping stars like our sun. These days Hertzsprung-Russell diagrams are used to present stellar evolution in pictures to students. They're not used much any more for developing new scientific theories.
On a Hertzsprung-Russell diagram, our Sun is plotted very close to the middle of the main sequence at the intersection of luminosity 1 and temperature 5780K. Therefore, the sun is class G or a "yellow star").
Seabird
Seabirds are birds that have adapted so they are better able to live at sea or near it. Many seabirds live "at sea", that is, far away from land. They may only come on land to breed. Other seabirds live in colonies on islands. Very often, seabirds use the sea for food, most often fish or shellfish. The first seabirds evolved in the Cretaceous period, and modern seabird families first appeared in the Palaeogene. The similarities between them are examples of convergent evolution. The same environmental problems and feeding niches have resulted in similar adaptations.
Seabirds share a number of adaptations to sea life. They live longer, breed later and have fewer young than other birds. They do spend a great deal of time with their young. Most species nest in colonies. These vary from a few dozen birds to millions. Many species take long annual migrations every year, crossing the equator or circumnavigating the Earth in some cases. They feed both at the ocean's surface and below it, and even feed on each other. Seabirds vary in how much of the year they spend at sea.
Tropical Depression One (2009)