Highlights of Astronomy

from Main Sequence Stars.- Objective-Prism Radial Velocities at High Latitudes.- Discussion of the Calculation of the Density Law (Dz).- Motions of Near-Polar K-Giants Along the z Coordinate.- General Discussion of Topics in Part Two.- Three Summary and Conclusions - Present Results and Future Problems for Study.- The Role of Proper Motions in Determining the Luminosity and Density Functions.- Concluding Remarks Part Two.- Current Results and Suggestions for Future Work.- 5. Stellar Atmospheres as Indicator and Factor of Stellar Evolution.- Introduction-Observational Evidence.- Introductory Talk.- Observational Evidence for Atmospheric Physical Characteristics Relevant to Stellar Evolution.- Behaviour of Microturbulence with Evolution.- Observational Evidence for Atmospheric Chemical Composition Peculiarities Relevant to Stellar Evolution.- Stellar Atmospheres as Boundary Condition of Internal Structure.- Sensitivity of Internal Structure to the Surface Boundary Condition.- Boundary Conditions with Mass Loss: General Considerations.- Mass Loss in Stars of Moderate Mass by Stellar Winds and Effects on the Evolution.- Boundary Condition with Mass Loss: The Radiatively-Driven Wind Model.- Alteration of Surface Chemical Composition of Stars by Transport Phenomena.- Stratification of Elements in a Quiet Atmosphere: Diffusion Processes.- Competition Between Diffusion Processes and Hydrodynamical Instabilities in Stellar Envelopes.- Alteration of Surface Chemical Composition of Stars by Nuclear Reaction.- Mixing Between Burned Core Material and Surface Layers.- Decay of Light Elements in Stellar Envelopes.- Conclusion.- 6. The Small Scale Structure of Solar Magnetic Fields.- Observations of Small-Scale Photospheric Magnetic Fields.- Small Scale Solar Magnetic Fields: Theory.- Some Comments on the Measurement of Small Scale Strong Magnetic Fields on the Sun.- Line Profiles of Faculae and Pores.- Facular Models, the K-Line, and Magnetic Fields.- Small Magnetostatic Flux Tubes.- Flows in Magnetic Flux Tubes.- Discussion.- Concluding Remarks.- 7. The Impact of Ultraviolet Observations on Spectral Classification.- Present Status of Spectral Classification in the Conventional Wavelength Range with Emphasis Upon Early-Type Stars.- Spectral Classification of Early-Type Stars from the Low Dispersion Ultraviolet Spectra.- Spectral Classification of B and A Stars from the Line Features of S2/68 Spectra.- Behaviors of B Star Continua and Absorption Features Determined from the TDl S2/68 "Ultraviolet Bright Star Spectrophotometric Catalogue" and from Copernicus Spectra.- Discussion.- Spectral Classification Using ANS Photometric Data.- Spectral Classification with Objective-Prism Spectra from Skylab.- Discussion.- An Atlas of Ultraviolet Stellar Spectra.- A New Temperature Scale for B Stars Based on OAO-2 Data.- Extreme Ultraviolet Observations of White Dwarfs.- The Near Ultraviolet Spectrum of Fe III as a Classification Criterion.- A Catalogue of 0.2 Å Resolution Far-Ultraviolet Stellar Spectra Measured with Copernicus.- Spectral Classification from Copernicus Data.- The Ultraviolet Spectrum of ? Lyrae.- The Mg II Features Near 2800 Å and Spectral Classification.- Discussion.- Concluding Remarks.- Observational Evidence of the Heterogeneities of the Stellar Surfaces.- Heterogeneity of the Solar Atmosphere.- The Heterogeneity of Surfaces of Magnetic Ap Stars.- Starspots on by DRA-Type Stars.- Starspots on AR Lac Type Stars.- Direct Observations of the Heterogeneity of Supergiant Disks.- On the Spottedness and Magnetic Field of T TAU-Type Stars.