Stellar atmospheres : $b A contribution to the observational study of high temperature in the reversing layers of starsPayne-Gaposchkin, Cecilia
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Stellar atmospheres : $b A contribution to the observational study of high temperature in the reversing layers of stars
Payne-Gaposchkin, Cecilia
Astrophysics; Stars -- Spectra; Stars -- Temperature; Thesis (Ph. D.)
The empirical relations used in the estimation of spectroscopic
parallax should provide material for examining the simple pressure
effect, as they are derived from the ratio of two lines in the same
spectrum. Unfortunately the line ratios actually in use were selected
[Pg 146]
because they were convenient to measure, and gave (empirically)
consistent results, not for reasons of theoretical tractability.
Fourteen line ratios are used, for example, by Harper and Young,[421]
but only four of these consist of pairs of unblended lines with known
series relations. It is only for such lines that a useful test of
theory can be made.
TABLE XXIII
M
=
+7
+8.8
+9.2
+11.0
+13.2
+6
+13.3
+5
+3.5
+5.0
+7.4
+9.6
+4
+10.0
+10.8
+3
-1.8
+0.5
+3.8
+6.7
+2
+6.7
+7.0
+7.6
+10.0
+1
-7.2
-3.8
+0.2
+3.2
0
+3.5
+3.4
+3.2
+3.0
1
-12.9
-8.2
-3.2
-0.3
-2
+0.3
-0.2
-1.4
-3.7
-3
-12.1
-7.3
-3.8
-4
-2.8
-4.2
-5.8
-10.0
M
=
+6
-2.0
-1.4
+5
-1.5
-0.5
0.0
+1.0
+4
+1.2
+1.3
+3
+1.8
+3.3
+4.4
+4.5
+2
+5.0
+3.0
+1
+4.8
+6.5
+7.8
+7.6
0
+6.5
+4.7
-1
+8.6
+9.3
+11.0
+11.0
-2
+12.0
+8.6
+8.6
+8.2
M
=
+6
-18.1
+5
-3.7
-5.8
-9.6
-14.7
+4
-15.3
+3
-1.0
-3.3
-6.6
-11.0
+2
-12.4
+1
+1.7
-0.6
-3.7
-7.5
0
-9.4
-1
+4.5
+2.0
-0.9
-4.0
-2
-6.6
-3
+7.2
+4.7
+2.0
-0.2
M
=
+6
+7.4
+6.2
+5
+6.2
+4
+4.3
+3.0
+3
+3.0
+2
+1.3
0.0
+1
0.0
0
0.0
-2.0
1
+2.6
-2
+2.0
+0.7
-3
+5.2
[Pg 147]
The preceding table contains a transcription of the reduction-curve
material given by Harper and Young for the four pairs of lines
mentioned. Tabulated quantities are the “step differences” for the
classes at the heads of the columns, and the absolute magnitudes
contained in the first column.
Presumably the irregularities of the observed curves have been smoothed
out in forming the reduction table, but the figures will certainly give
an indication of the direction in which a given line is affected by
absolute magnitude.
The predicted effect of lowered pressure upon the lines involved is
contained in the table that follows:
Line
Source
Max.
Effect of lowered pressure
4071
Fe (sub)
weakened throughout
4077
Sr+ (ult)
strengthened in , weakened in and
4215
Sr+ (ult)
strengthened in , weakened in and
4247
Sc+ (?)
strengthened throughout range
4250
Fe (sub)
weakened throughout
4455
Ca (sub)
weakened throughout
4494
Fe (sub)
weakened throughout
The predicted changes in the line ratios with lowered pressure are
therefore as follows:
Public-domain text, read in full here on John Shaqi.
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