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.)
In the special case where , the second
curve, which represents the growth of the fraction , becomes
a straight line parallel to the temperature axis, and the first, or
ionization, curve, approaches the zero ordinate asymptotically at low
temperatures. The ordinate of the curve representing is zero,
and the resultant sum gives a curve identical with the curve for the
ultimate lines. Ultimate lines thus appear as the special case of
subordinate lines for which the excitation potential is zero. This fits
exactly with the definition of ultimate lines as the lines naturally
absorbed by the cold vapor—no initial excitation is required to bring
the atoms into a state in which they can absorb.
LINES OF IONIZED ATOMS
[Pg 102]
As soon as ionization sets in, the absorbing layer begins to
contain a new kind of atom, derived from the neutral atoms by
the complete ejection of one electron. These ionized atoms will
absorb their own spectrum, which differs completely from that
of the corresponding neutral atom; and the degree of absorption
will again depend on the number of such ionized atoms present
in the reversing layer.
The ionized atom has in general a spectrum corresponding
exactly to that of the neutral atom preceding it in the periodic
table, but with a different Rydberg constant.[368][369] Two types of
lines arise, as before—ultimate and subordinate lines. For
the number of atoms which can absorb the ultimate lines of the
enhanced spectrum, the formula reduces to
Account is here taken of the residual neutral atoms by the
middle term of the denominator, which is very small, and is
only of sensible magnitude for the ultimate lines, when the
numerator is equal to unity.
Figure 7
Maximum of the ultimate line of an ionized atom. Ordinates are
logarithms of computed fractional concentrations; abscissae are
temperatures in thousands of degrees. The curve is drawn for
the line 4554 of Ba+, on the assumption that is
.
The following curve shows the number of absorbing atoms. The flatness
of the maximum is especially to be noted, suggesting that the ultimate
lines of the ionized atom, like the ultimate lines of the neutral
[Pg 103]
atom, will be very persistent. The and lines of Ca+, and
the corresponding lines 4077 and 4215 of Sr+, and 4555 of Ba+, would
thus be expected to show over a considerable range in temperature and
spectrum, and this is actually found to be the case.
Public-domain text, read in full here on John Shaqi.
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