| 1. | The emission line spectrum associated with dense stellar winds has persisted ever since the late 19th century.
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| 2. | Soon I was using phrases like " event horizon " and " dark-line spectrum " with ease.
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| 3. | :: : Those nebula are emission nebulas wich emit light at particular wavelengths in a line spectrum.
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| 4. | One has the emission-line spectrum of a WC7 Wolf-Rayet star, while the other is a B0 giant.
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| 5. | The source image is reimaged, every point, as a line spectrum on what is called a detector-array column.
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| 6. | It was even classified as a Wolf-Rayet star because of its strong emission line spectrum, and named WR 101f.
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| 7. | Therefore, flat-line spectrums in general are often referred to as white, whether they represent light or something else ."
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| 8. | The emission line spectrum is produced in the dense stellar wind and little is known about the underlying photosphere.
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| 9. | Medium-pressure UV lamps have a broad and pronounced peak-line spectrum and a high radiation output but lower UVC efficiency of 10 % or less.
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| 10. | Later advancements in technology allowed for even more stacking on the Type L-5E, allowing 22 mastergroups to be stacked into a 66 MHz line spectrum.
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