Stellar atmospheres : $b A contribution to the observational study of high temperature in the reversing layers of starsPayne-Gaposchkin, Cecilia
Science
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.)
Ultimate lines of neutral atoms. Ordinates are logarithms of computed
fractional concentrations; abscissae are temperatures in thousands of
degrees. The curves show the decrease in the number of neutral atoms,
with rising temperature, and the consequent decay in strength of the
ultimate lines, for the atoms indicated on the right margin.
As ionization becomes more and more complete, the intensity of the
ultimate lines falls off until so small a number of neutral atoms
remains that their lines cease to appear in the absorption spectrum.
SUBORDINATE LINES
The neutral atom gives rise to other lines besides the ultimate
lines, but these require the transfer of an electron from some
stationary state, not the normal one, to another stationary state.
The atom must receive a definite quantity of energy, equal to the
excitation potential of the initial stationary state, in order to
be in a condition to absorb a line of a subordinate
[Pg 100] series which
originates from that state. If there is an appreciable energy supply,
a certain fraction of the neutral atoms present will have received
this excitation energy, which is of course smaller than the ionization
potential, and these atoms will be in a position to absorb the
subordinate series.
Figure 6
Production of the maximum of an absorption line. Ordinates are
logarithms of computed fractional concentrations; abscissae are
temperatures in thousands of degrees. The curves reproduced are those
for the Mg + line at 4481. The upper broken curve represents the
fraction of magnesium atoms that is singly ionized at the corresponding
temperature; the lower broken curve represents the fraction of the Mg +
atoms present that is in a suitable state for the absorption of 4481.
The full line represents the sum of the ordinates of the dotted curves,
and gives the fraction of the total number of magnesium atoms that
is able to absorb 4481 at the various temperatures indicated by the
abscissae.
The fraction, , of the total number of neutral atoms which have
[Pg 101]
become able to absorb the lines associated with a definite excitation
potential is given by Fowler and Milne as
where () = excitation potential. The quantity
increases with the temperature, approaching the value unity
asymptotically.
The total number of atoms active in absorbing a subordinate series
at any temperature is evidently the product of the number of
neutral atoms and the quantity . The curves for these
two quantities are plotted logarithmically in Figure 6, the magnesium
line 4481 being used as an illustration. The total number of absorbing
atoms may be obtained by adding the ordinates. It will be seen that the
number of such atoms increases, passes through a maximum and decreases
again, as the temperature is raised. The maximum for a subordinate
line of the neutral atom may occur, as in the case of helium, when
ionization is far advanced.
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