Ratio of horizontal branch stars to red giant stars in globular clusters
Horizontal branch and red giant stars ratio estimated in globular clusters for He abundance
Iben, I., Jr.↗
Engineering topics
Strom, S. E.
Publications and source records attributed to Strom, S. E..
Observational results concerning departures from LTE in late B stars
LTE departures in late B stars from measurements of Balmer and Paschen discontinuities
Smith, M. A.↗
Possible variations of helium content with position in the galaxy
Variation of helium abundance with galactic position of stars
Shipman, H. L.↗
An analysis of the peculiar A star HD 204411.
Model atmosphere analysis of line identifications and equivalent width data for relatively cool Ap star HD 204411, discussing atmospheric composition
Sargent, W. L. W.↗
Departures from LTE in the hydrogen lines of late B stars.
Atomic hydrogen departures from LTE computed for models of B star atmospheres, assuming detailed balance in hydrogen lines
Peterson, D. M.↗
Model atmospheres for RR Lyrae stars.
RR Lyrae gap stellar model atmospheres including radiation spectra, temperature radiation and convection, etc
Strom, S. E.↗
The effect of Lyman-alpha wing opacity on the temperature scale and helium content for subdwarfs.
Lyman alpha wing opacity effect on temperature scale and helium content in F and G subdwarf atmospheres
Strom, K. M.↗
The use of model atmospheres in the interpretation of stellar spectra
H-R diagram stellar spectra interpretation using model atmospheres describing temperature, gravity and chemical composition
Strom, S. E.↗
Luminosity effects in the Balmer lines of early-type stars
Luminosity effects in Balmer lines of early type stars, noting H alpha equivalent width decrease
Peterson, D. M.↗
An analysis of the peculiar A star HD 204411
Spectrum analysis of cool Ap star HD 204411
Sargent, W. L. W.↗
The early A stars. III - Model-atmosphere abundance analysis of four field stars.
Element abundances of sharp lined field early A stars using model atmosphere
Conti, P. S.↗
Surface-gravity determinations for main- sequence B stars.
Main sequence B stars surface gravity determinations from comparison between model atmosphere computed and observed H gamma line equivalent widths
Peterson, D. M.↗
On the variation of the microturbulence parameter with chemical composition.
Microturbulent velocity parameter correlation to iron-to-hydrogen ratio for G dwarfs, using model atmosphere abundance analyses
Strom, S. E.↗
The early A stars. II - Model-atmosphere abundance analysis of eight stars in the Pleiades.
Anomalously low Sc/Sr ratio in A zero stars of Pleiades cluster from model atmosphere abundance analysis
Conti, P. S.↗
On the composition of Sirius revisited
Model atmosphere analysis to determine abundances, in stellar structures
Gingerich, O.↗
Analysis of F and G subdwarfs. II - A model-atmosphere abundance analysis of the subdwarfs HD 140283 and HD 19445.
Model atmospheres utilization for abundance analysis of Population 2 F and G subdwarf stars, noting convection role in atmospheric temperature structures
Cohen, J. G.↗
On the variation of the microturbulence parameter with chemical composition
Stellar model atmosphere abundance analysis to correlate microturbulent velocity parameters with iron to hydrogen ratio for G dwarfs
Strom, S. E.↗