Content About: Structure and Evolution of Stars
New stellar plasma density determinations by the GHRS: The transition regions of Capella and Gamma Draconis
Evolution of Single Stars. I. Stellar Evolution from Main Sequence to White Dwarf or Carbon Ignition
Spectroscopic studies of Wolf-Rayet stars with absorption lines. I - The probable single WN5 star HD 193077
Pulsar radiation patterns. V - Synopsis of results and conclusions concerning the physical mechanism
Activity‐related Changes in Local Solar Acoustic Mode Parameters from Michelson Doppler Imager and Global Oscillations Network Group
Far-Ultraviolet Continuum Emission: Applying this Diagnostic to the Chromosphers of Solar-Mass Stars
Coronae of Nondegenerate Single and Binary Stars. A Survey of Our Present Understanding and Problems Ripe for Solution
A recalibration of the quiet Sun millimeter spectrum based on the Moon as an absolute radiometric standard
A Critical Evaluation of Temperature Determinations in the Low Solar Chromosphere as Obtained from the Ultraviolet Continuum Data
Sensitivity of inferred subphotospheric velocity field to mode selection, analysis technique and noise
What Can Solar and Stellar Ultraviolet Observations Tell About Chromospheric and Coronal Heating Mechanisms?
Erratum: "Evidence for a corona of Beta Geminorum" [Astrophys. J., Lett., Vol. 193, p. L107 - L110 (1974)].