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They were distinguished and named by Walter Baade (1893–1960).
¿ Puedes sacarnos de aquí?HechoLiterature Literature
In Herr Meyer's dream in Chap. 3 we have already made use of Walter Baade's findings.
James BaylorLiterature Literature
Walter Baade, in his late fifties, had lost none of his fondness for astronomical puzzle-solving.
Si.Gracias, cariñoLiterature Literature
His first choice candidate as his follower was Walter Baade who refused because of better astronomical working conditions at the Californian Mt.
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Nine of these variables were reported by German astronomer Walter Baade in 1928, and the tenth by American astronomer Helen Sawyer in 1946.
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In 1944 Walter Baade confirmed dwarf ellipticals NGC 147 and NGC 185 as members of the Local Group by resolving them into individual stars, thanks to their relatively little distance.
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Walter Baade successfully petitioned the Hamburg senate to have Schmidt camera installed in 1937, and it was completed in 1954 after work restarted on in 1951 after being interrupted by WWII.
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The term was first coined by Walter Baade and Fritz Zwicky in 1931.
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In 1928, his compatriot Walter Baade used the more powerful 2.5-metre telescope at the Mount Wilson Observatory in California to successfully make out its individual stars.
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The two were named after the Portuguese explorer, Ferdinand Magellan. Each telescope is also named; the Baade after astronomer Walter Baade, and the Clay after the philanthropist Landon T. Clay.
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In the 1940s, a German astronomer named Walter Baade took advantage of the blackouts that were ordered in response to potential attacks during World War II and used the Mt.
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The spiral arms of the Andromeda Galaxy are outlined by a series of HII regions, first studied in great detail by Walter Baade and described by him as resembling "beads on a string".
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1954: The Hubble Constant tumbles from 558 to 280 when Walter Baade shows that Hubble had unknowingly used two distinct populations of stars - with different relationships between pulsation rate and light output - to calibrate distance.
Las aguas delimitadas por una línea que comienza enel punto situado a #° #′ de latitud norte, #° #′ de longitud oeste; después con rumbo oeste hasta los #° #′ de longitud oeste; después con rumbo sur hasta los #° #′ de latitud norte; después con rumbo este hasta los #° #′ de longitud oeste; después con rumbo norte hasta el punto de partidaParaCrawl Corpus ParaCrawl Corpus
The observation of recent star formation in the galaxy NGC 187 contradicts the scheme established in the 1940s by the distinguished astronomer Walter Baade according to which dwarf elliptical galaxies are populated only by old stars.
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The two telescopes are named after the astronomer Walter Baade and the philanthropist Landon T. Clay. First light for the telescopes was on September 15, 2000 for the Baade, and September 7, 2002 for the Clay.
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This is because these galaxies were directly involved in the construction of one of the key paradigms of the astrophysics of this century: the concept of stellar populations, introduced by Walter Baade (1893- 1960), an astronomer at the Carnegie Institute in Pasadena (California, USA).
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The idea that European astronomers should establish a common large observatory was broached by Walter Baade and Jan Oort at the Leiden Observatory in the Netherlands in spring 1953.[10] It was pursued by Oort, who gathered a group of astronomers in Leiden to consider it on June 21 that year.
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In 1934, Walter Baade and Fritz Zwicky proposed the existence of the neutron star,[21][22] only a year after the discovery of the neutron by Sir James Chadwick.[23] In seeking an explanation for the origin of a supernova, they proposed that the neutron star is formed in a supernova.
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His measurement demonstrated conclusively that this feature was not a cluster of stars and gas within our own galaxy, but an entirely separate galaxy located a significant distance from the Milky Way.[29] In 1943, Walter Baade was the first person to resolve stars in the central region of the Andromeda Galaxy.
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This episode describes the important steps in the creation of ESO, from an early meeting on a boat trip in the Netherlands in June 1953, when the astronomers Walter Baade and Jan Oort told colleagues about their plan for a European observatory in the southern hemisphere, to the final signature of the ESO convention on 5 October 1962 by five European countries (Belgium, Germany, France, the Netherlands and Sweden).
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20 sinne gevind in 8 ms. Hulle kom uit baie bronne en word nie nagegaan nie.