Wolf–Rayet stars, often abbreviated as WR stars, are a rare heterogeneous set of stars with unusual spectra showing prominent broad emission lines of ionised helium and highly ionised nitrogen or carbon. The spectra indicate very high surface enhancement of heavy elements, depletion of hydrogen, and … See more In 1867, using the 40 cm Foucault telescope at the Paris Observatory, astronomers Charles Wolf and Georges Rayet discovered three stars in the constellation Cygnus (HD 191765, HD 192103 and HD … See more The separation of Wolf–Rayet stars from spectral class O stars of a similar temperature depends on the existence of strong emission lines of ionised helium, nitrogen, carbon, … See more Wolf–Rayet stars are a normal stage in the evolution of very massive stars, in which strong, broad emission lines of helium and nitrogen ("WN" … See more A Wolf–Rayet galaxy is a type of starburst galaxy where a sufficient number of WR stars exist that their characteristic emission line spectra become visible in the overall spectrum of the galaxy. Specifically a broad emission feature due to the 468.6 nm He ii and … See more Wolf–Rayet stars were named on the basis of the strong broad emission lines in their spectra, identified with helium, nitrogen, carbon, silicon, and oxygen, but with hydrogen lines usually weak or absent. The first system of classification split these into stars with … See more The first three Wolf–Rayet stars to be identified, coincidentally all with hot O-class companions, had already been numbered in the HD catalogue. These stars and others … See more A significant proportion of WR stars are surrounded by nebulosity associated directly with the star, not just the normal background nebulosity associated with any massive star forming region, and not a planetary nebula formed by a post-AGB star. The nebulosity … See more WebMar 14, 2024 · This is a Wolf-Rayet star, one of the most luminous, massive and briefly detectable stars known. It's in the process of casting off outer layers before going supernova. WR 124 is 30 times the mass of the Sun and has shed 10 Suns’ worth of material so far. nasa.gov.
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WebOct 8, 1997 · The star may represent the short-lived "missing link" between normal hot stars and the exotic Wolf- Rayet stars which have lost their outer layers. This transitional phase is so rare that the Pistol Star would be only the seventh of its kind in the Galaxy. Weighing in at 100 to 200 times the mass of the Sun when it began life, the Pistol Star ... sacs commission on colleges
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WebFeb 7, 2024 · ABSTRACT. We provide line luminosities and spectroscopic templates of prominent optical emission lines of 133 Galactic Wolf–Rayet (WR) stars by exploiting Gaia DR3 parallaxes and optical spectrophotometry, and provide comparisons with 112 counterparts in the Magellanic Clouds. Average line luminosities of the broad blue (He ii … WebA catalog of northern Wolf-Rayet Stars and the Central Stars of Planetary Nebulae. Name RA DEC Epoch Sp Type Mag Comments HD826 00:13:01 72:31:20 2000 WC/CSPN 11 … WebSep 23, 2024 · The hottest known star, WR 102, is one such Wolf-Rayet, sporting a surface temperature more than 35 times hotter than the Sun. Like Baskin-Robbins, Wolf-Rayet stars come in a variety of flavors. ischiofemoral interval injection cpt