Walter Baader
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Populations I and II…1950s by the German-born astronomer Walter Baade. The members of these stellar populations differ from each other in various ways, most notably in age, chemical composition, and location within galactic systems.
Read More…1950s by the German-born astronomer Walter Baade. The members of these stellar populations differ from each other in various ways, most notably in age, chemical composition, and location within galactic systems.
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Milky Way GalaxyPrincipal population typesIn 1944 the German-born astronomer Walter Baade announced the successful resolution into stars of the centre of the Andromeda Galaxy, M31, and its two elliptical companions, M32 and NGC 205. He found that the central parts of Andromeda and the accompanying galaxies were resolved at very much fainter magnitudes than…
Read MoreIn 1944 the German-born astronomer Walter Baade announced the successful resolution into stars of the centre of the Andromeda Galaxy, M31, and its two elliptical companions, M32 and NGC 205. He found that the central parts of Andromeda and the accompanying galaxies were resolved at very much fainter magnitudes than…
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galaxyThe distance to the Andromeda Nebula…1944 did the German-born astronomer Walter Baade finally resolve the bulge of M31. Using red-sensitive plates and very long exposures, he managed to detect the brightest red giants of this old population. Out in the arms there exist many young, bright, hot blue stars, and these are easily resolved. The…
Read More…1944 did the German-born astronomer Walter Baade finally resolve the bulge of M31. Using red-sensitive plates and very long exposures, he managed to detect the brightest red giants of this old population. Out in the arms there exist many young, bright, hot blue stars, and these are easily resolved. The…
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