Electron excitation of forbidden lines occurring in gaseous nebulae

MJ Seaton - Proceedings of the Royal Society of London …, 1953 - royalsocietypublishing.org
In a previous paper the Hartree-Fock method has been used to calculate electron excitation
cross-sections for the ground configuration terms of O I. In the present paper the …

Quantum defect theory

MJ Seaton - Molecular Applications of Quantum Defect Theory, 2019 - taylorfrancis.com
Quantum defect theory (qdt) is concerned with the properties of an electron in the field of a
positive ion and, in particular, with expressing those properties in terms of analytical …

Thermal inelastic collision processes

MJ Seaton - Symposium-International Astronomical Union, 1958 - cambridge.org
Section II contains a summary of relevant collision theory methods. Section III is concerned
with heavy particle collisions: excitation of H 1s hyperfine structure (hfs) states by H atom …

The Ionization Structure of Planetary Nebulae: V. Radii, Luminosities and Problems of Evolution

MJ Seaton - Monthly Notices of the Royal Astronomical Society, 1966 - academic.oup.com
The forty-seven planetaries of Paper IV are divided into two Classes:(a) with He II lines and
(b) without He II lines. From results obtained in IV, the ionized hydrogen mass M of Class (a) …

The quantum defect method

MJ Seaton - Monthly Notices of the Royal Astronomical Society, 1958 - academic.oup.com
Summary The Quantum Defect Method uses interpolated or extrapolated quantum defects to
determine the asymptotic forms of atomic wave functions. The method may be used in the …

Excitation of coronal lines by proton impact

MJ Seaton - Monthly Notices of the Royal Astronomical Society, 1964 - academic.oup.com
Cross sections are calculated for the transition| $\text {Fe}^{+ 13}\enspace
3p\frac12\rightarrow3p\frac32 $| produced by proton impact. The excitation rate increases …

Opacities for stellar envelopes

MJ Seaton, Y Yan, D Mihalas… - Monthly Notices of the …, 1994 - academic.oup.com
We define stellar envelopes to be those regions of stellar interiors in which atoms exist and
are not markedly perturbed by the plasma environment. Availability of accurate and …

Use of the R matrix method for bound-state calculations. I. General theory

MJ Seaton - Journal of Physics B: Atomic and Molecular Physics, 1985 - iopscience.iop.org
In the close-coupling (CC) method of electron-atom collision theory, wavefunctions Psi E for
a system containing (N+ 1) electrons are expanded in terms of products of N-electron'target' …

The theory of excitation and ionization by electron impact

MJ Seaton - Atomic and molecular processes, 1962 - books.google.com
Consider the i—> collision to be of de-excitation type< v,). According to (6), when v,-is small,
10 becomes large for all finite L. One would expect P,,~(L) to go to zero as v,-goes to zero. In …

On the interpretation of radio recombination line observations

M Brocklehurst, MJ Seaton - Monthly Notices of the Royal …, 1972 - academic.oup.com
SUMMARY A substantial amount of data from atomic physics is required for the
interpretation of radio recombination line observations. A critical review of the available data …