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FUN THINGS TO DO
FUN THINGS TO DO

... out the stars at night. What constellations would the dinosaurs have seen back then? They would be different ones from those we see now! ...
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Lecture 17: Black Holes
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... Abstract. DG Tau is a classical T Tauri star showing an unusual X-ray spectrum, best described by two thermal components with different absorption columns. The soft X-rays are less absorbed than the hard X-rays, presumably coronal, component. This rules out stellar accretion as the origin of the sof ...
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... scientists believed that the relative abundance of elements in the atmospheres of the Sun and the stars was similar to that in Earth’s crust. In 1889, geochemist Frank Wigglesworth Clarke’s The Relative Abundance of the Chemical Elements was the result of his comprehensive sampling of minerals from ...
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... obtained should be corrected for by dividing it by the cosine L. The observational material for this exercise consists of two spectrograms of Arcturus taken about one half year apart on July 1, 1939 (a) and on January 19, 1940 (b). From the spectrum of (a) we can get VA and from (b) we can get VB. T ...
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R136a1



RMC 136a1 (usually abbreviated to R136a1) is a Wolf-Rayet star located at the center of R136, the central condensation of stars of the large NGC 2070 open cluster in the Tarantula Nebula. It lies at a distance of about 50 kiloparsecs (163,000 light-years) in the Large Magellanic Cloud. It has the highest mass and luminosity of any known star, at 265 M☉ and 8.7 million L☉, and also one of the hottest at over 50,000 K.
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