NGC 2080, the Latvian word for horn. (The Daugava River makes a horn shaped turn in the Ķengarags area.) Present. Ķengarags consists of three neighborhoods, known as Ķengarags, Ķengarags-2, and Ķengarags-3 from the north (center of Riga) to the south (outskirts) respectively. Each of these parts of Ķengarags consists of both residential and commercial areas. The main streets of Ķengarags are Lokomotīves iela and Maskavas iela bordering Ķengarags on the east and west respectively. There are several public transport links with central Riga in Ķengarags. The train stations on the railway line within Ķengarags are Jāņavārti, Daugmale and Šķirotava stations. The PV 	Ķengarags
4065982	train service uses the Riga-Moscow railway. From Riga Central Train Station by train it takes about 15 minutes. An alternative would be either route 7 or 9 tram which follows Maskavas iela and terminates at the Dole supermarket. The most commonly used method of Ķengarags residents to get to city center is the route 15 trolleybus, which runs through residential neighborhoods and terminates at the southern tip of Ķengarags on Višķu iela. The residential areas of Ķengarags consist of private houses and apartment buildings, consisting of 4, 5, 9, and 12-story buildings. Most apartments have cable television which 	Ķengarags
4065983	was installed in the last years of the Soviet period. Most other Riga neighborhoods receive their television programs through on-roof antennas. The residents of Ķengarags also benefit from the proximity of the Daugava river which is within walking distance for many people. Ķengarags Ķengarags is a neighborhood in the city of Riga, Latvia. It is located in the southern part of the city. Ķengarags borders the Daugava River to the west, the Riga-Moscow railway line to the east, Rumbula to the south, and Krasta Residential Neighborhood to the north. History. Ķengarags was the location of a Sword Brothers 	Ķengarags
4065984	NGC 2080 NGC 2080 NGC 2080 (The Ghost Head Nebula") is a star-forming region and emission nebula to the south of the 30 Doradus (Tarantula) nebula, in the southern constellation Dorado. It belongs to the Large Magellanic Cloud, a satellite galaxy to the Milky Way, which is at a distance of 168,000 light years. NGC 2080 was discovered by John Frederick William Herschel in 1834. The Ghost Head Nebula has a diameter of 50 light-years and is named for the two distinct white patches it possesses, called the "eyes of the ghost". The western patch, called A1, has a bubble  in the center which was created by the young, massive star it contains. The eastern patch, called A2, has several young stars in a newly formed cluster, but they are still obscured by their originating dust cloud. Because neither dust cloud has dissipated due to the stellar radiation, astronomers have deduced that both sets of stars formed within the past 10,000 years. These stars together have begun to create a bubble in the nebula with their outpourings of material, called stellar wind. The presence of stars also greatly influences the color of the nebula. The western portion of the nebula  has a dominant oxygen emission line because of a powerful star on the nebula's outskirts; this colors it green. The rest of the nebula's outskirts have a red hue due to the ionization of hydrogen. Because both hydrogen and oxygen are ionized in the central region, which appears pale yellow; when hydrogen is energized enough to emit a second wavelength of light, it appears blue, as in the area surrounding A1 and A2. NGC 2080 should not be confused with the Ghost Nebula (Sh2-136) or the Little Ghost Nebula (NGC 6369). NGC 2080 NGC 2080 (The "Ghost