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STATISTICAL LINE BLANKETING IN ARCTURUS I. BLANKETING-COEFFICIENT DESCRIPTION OF OBSERVATIONS
FRANK N. EDMONDS, JR.
Publications of the Astronomical Society of the Pacific
Vol. 85, No. 503 (February 1973), pp. 24-41
Published by: Astronomical Society of the Pacific
Stable URL: http://www.jstor.org/stable/40675329
Page Count: 18
You can always find the topics here!Topics: Wavelengths, Statistical interpretations, Telluric lines, Rum, Line spectra, Statistical models, Carbon, Musical intervals, Sun, Assembly lines
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A statistical description of line blanketing is presented for Arcturus (α Boo, K2 IIIp, v = + 0.06) which is based on equivalent widths and identifications of roughly 10,000 spectral lines within the wavelength region λλ3600-25,000 Å. Equivalent-width contributions or blanketing coefficients for lines grouped as to equivalent width and identification are given for 100 Å wavelength intervals for λ < 9000 Å and 500 Å intervals for λ > 9000 Å (Tables I and II). Strong lines are listed individually (Table III), and the variation or scatter of blanketing within intervals is described. Corrections to this description for limitations in the observations and their analysis are discussed.
Publications of the Astronomical Society of the Pacific © 1973 The University of Chicago Press