Ultraviolet Stellar Spectra and Related Ground-Based Observations [Paperback]

I / Stellar Fluxes.- A. Absolute Calibration.- 1. Absolute intensity calibration methods in the vacuum UV region.- 2. An investigation of the properties of vacuum-ultraviolet radiation detectors (Abstract).- 3. Recent absolute calibration work at Palomar Mountain.- 4. General discussion (On calibration methods).- B. Interstellar Extinction.- 1. Interstellar extinction (Introductory lecture).- 2. Ultraviolet interstellar extinction from a comparison of ? Persei and ? Pesei.- 3. Observations of interstellar extinction in the ultraviolet with the OAO satellite.- 4. On dielectric models of interstellar grains.- 5. Extinction curves for graphite-silicate grain mixtures.- 6. Measurement of interstellar extinction in emission line stars.- 7. The interstellar extinction curve from 4000 ? to 6500 ?.- C. Theoretical Models for Stellar Fluxes.- 1. The effective temperatures of the O stars.- 2. The effect of Silicon and Carbon opacity on ultraviolet stellar spectra.- D. Observed Stellar Fluxes.- 1. Review of ultraviolet and visual continuum observations and comparisons with models.- 2. The stellar temperature scale from 05 to A0.- 3. On ultraviolet fluxes, bolometric corrections and effective temperatures of late B to F stars.- 4. Far-ultraviolet intensities of Orion stars.- 5. Ultraviolet photometry of stars obtained with the Celescope experiment in the Orbiting Astronomical Observatory.- 6. Photographic magnitudes of 201 stars at 2600 ?.- 7. Spectrophotometrie integree des galaxies proches dans lultraviolet (exp?rience Pers?e).- 8. Low resolution stellar spectrophotometrie observations in the region 1500 ?3000 ?.- 9. Absolute stellar photometry in the region 1200 ?3000 ?.- 10. Preliminary note on the astronomical satellite Kosmos 215.- 11. Ultraviolet photometry of stars from OSO II.- 12. The ultraviolet solar opacity.- II / Stellar Line Spectra.- A. Rocket and Satellite Observations of Ultraviolet Spectra.- 1. Observations of ultraviolet stellar spectra.- 2. PhotoelectriclS!