The Astrophysical Journal 23
The Astrophysical Journal 23
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i), or Uke an inverted fl (Fig. 2). The former has diflFuse wings, a bright center, and disappears as a. very narrow line. The latter is broad Fig. I M Fig. 2 The iron lines reverse some- and uniform in brightness, has barely perceptible wings, and dis- appears as a ribbon of light. Cu X 5218 is characteristic of the former, Cu X 5104 of the latter type, what as shown in Fig. 3. They twin at an early stage, appearing exactly like a pair of adjacent lines with very sharp edges. As the in- tensit...y is increased, the components retreat from each other, broaden, and finally show reversal proper. The figures exaggerate the actual effects and ignore second-order phenomena like superposed structures; but only the effects shown are to be dis- cussed in this paper.
The resolving power of an echelon grating is sufficient to justify considerable detail in the description of the structure of a Une 0.2 t.-m. broad. An echelon of thirty plates, each 10 mm thick and differing in width by J mm from its neighbors, has a dispersion approximately the same as that of a 21 -foot grating in the second order.
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To quickly assess the difficulty of the text, read a short excerpt:
i), or Uke an inverted fl (Fig. 2). The former has diflFuse wings, a bright center, and disappears as a. very narrow line. The latter is broad Fig. I M Fig. 2 The iron lines reverse some- and uniform in brightness, has barely perceptible wings, and dis- appears as a ribbon of light. Cu X 5218 is characteristic of the former, Cu X 5104 of the latter type, what as shown in Fig. 3. They twin at an early stage, appearing exactly like a pair of adjacent lines with very sharp edges. As the in- tensit...y is increased, the components retreat from each other, broaden, and finally show reversal proper. The figures exaggerate the actual effects and ignore second-order phenomena like superposed structures; but only the effects shown are to be dis- cussed in this paper.
The resolving power of an echelon grating is sufficient to justify considerable detail in the description of the structure of a Une 0.2 t.-m. broad. An echelon of thirty plates, each 10 mm thick and differing in width by J mm from its neighbors, has a dispersion approximately the same as that of a 21 -foot grating in the second order.
What to read after The Astrophysical Journal 23?
You can find similar books in the "Read Also" column, or choose other free books by University of Chicago to read onlineMoreLess
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