The Astrophysical Journal
The Astrophysical Journal
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In our eReader you can find the full English version of the book. Read The Astrophysical Journal Online - link to read the book on full screen. Our eReader also allows you to upload and read Pdf, Txt, ePub and fb2 books. In the Mini eReder on the page below you can quickly view all pages of the book - Read Book The Astrophysical Journal
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1.9 47 0.052 1.44 46 0.050 3-2 57 0.06a 2.6 56 0.062 4.7 66 0.072 3 9 64 0.071 6.7 76 0.084 50 69 0.076 9.5 93 0.102 6.0 72 0.079 12.9 109 0. 120 71 75 0.083 19.0 115 0.126 9.0 77 0.085 12.2 90 0.099 20.2 115 0. 126 y ' 8 y y M 6 y y & ^ > < c .^ y y y ^ y 6 X^ ^ 4 e •5 Intensity 5 10 Fig. 3.— Width: Intensity, He, X5876. Digitized by Google UNE STRUCTURE, III 117 The width of the line is seen to vary considerably with its inten- sity, more than doubling within the range available. The relation between width and intensity is approximately linear for low and moderate intensities. At great intensities the width is, if anything, less than this proportionality would indicate. At the intensity called 10, the capillary of the tube was just commencing to bum and show sodium lines, and possibly this might account for the falling-off from the linear relation at high intensities, but arc lines show a similar falling off. Plotting against a quadratic or logar- ithmic abscissa does not help matters.
What to read after The Astrophysical Journal?
You can find similar books in the "Read Also" column, or choose other free books by University of Chicago to read online
To quickly assess the difficulty of the text, read a short excerpt:
1.9 47 0.052 1.44 46 0.050 3-2 57 0.06a 2.6 56 0.062 4.7 66 0.072 3 9 64 0.071 6.7 76 0.084 50 69 0.076 9.5 93 0.102 6.0 72 0.079 12.9 109 0. 120 71 75 0.083 19.0 115 0.126 9.0 77 0.085 12.2 90 0.099 20.2 115 0. 126 y ' 8 y y M 6 y y & ^ > < c .^ y y y ^ y 6 X^ ^ 4 e •5 Intensity 5 10 Fig. 3.— Width: Intensity, He, X5876. Digitized by Google UNE STRUCTURE, III 117 The width of the line is seen to vary considerably with its inten- sity, more than doubling within the range available. The relation between width and intensity is approximately linear for low and moderate intensities. At great intensities the width is, if anything, less than this proportionality would indicate. At the intensity called 10, the capillary of the tube was just commencing to bum and show sodium lines, and possibly this might account for the falling-off from the linear relation at high intensities, but arc lines show a similar falling off. Plotting against a quadratic or logar- ithmic abscissa does not help matters.
What to read after The Astrophysical Journal?
You can find similar books in the "Read Also" column, or choose other free books by University of Chicago to read online
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