Ultraviolet Stellar Spectra and Related Ground-Based Observations
| Other Authors: | , |
|---|---|
| Format: | eBook |
| Language: | English |
| Published: |
Dordrecht
Springer Netherlands
1970, 1970
|
| Edition: | 1st ed. 1970 |
| Series: | International Astronomical Union Symposia
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| Subjects: | |
| Online Access: | |
| Collection: | Springer Book Archives -2004 - Collection details see MPG.ReNa |
Table of Contents:
- 1. Observations of ultraviolet stellar spectra
- 2. Photoelectric rocket spectra at 10 Å resolution (Abstract)
- 3. Rocket spectroscopy of ? Puppis below 1100 Å
- 4. Observations of strong stellar lines with the OAO
- 5. The far-ultraviolet spectrum of ? Cassiopeiae
- 6. UV spectrophotometry of Canopus from Gemini XI
- B. Ground-Based Observations of Spectra Relevant to the Ultraviolet
- 1. Review of ground-based observations of spectra relevant to the ultraviolet
- 2. Chromospheric activity in red giants, and related phenomena
- 3. Mass loss from early-type stars
- C. Theory Relevant to UV Spectra
- 1. A discussion of the theory for interpreting ultraviolet stellar spectra
- 2. Possibility of fluorescence phenomena in the ultraviolet spectrum of symbiotic stars and long period variables
- 3. Radiative acceleration and ultraviolet resonance line profiles in OB supergiants
- 4. Stellar-wind theory for O and B stars (Abstract)
- D. The Sun — a Typical G2V Star
- 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 Å
- 7. Spectrophotometrie integree des galaxies proches dans l’ultraviolet (expérience Persée)
- 8. Low resolution stellar spectrophotometrie observations in the region 1500 Å–3000 Å
- 9. Absolute stellar photometry in the region 1200 Å–3000 Å
- 10. Preliminary note on the astronomical satellite Kosmos 215
- 11. Ultravioletphotometry of stars from OSO II
- 12. The ultraviolet solar opacity
- II / Stellar Line Spectra
- A. Rocket and Satellite Observations of Ultraviolet Spectra
- 4. Lyman-? radiation from nebular objects
- Space and ground-based stellar spectrophotometry: a summary
- 1. Review of astrophysical conclusions from the UV solar spectra
- 2. Resonance lines in the solar chromosphere
- 3. On the contribution of solar activity to the ultraviolet spectrum of the Sun
- 4. Intensity distribution in the Lyman-? line at the solar limb
- 5. A high-resolution solar spectrum 2000 Å–2200 Å
- 6. Fabry-Pérot interferograms of the solar MgII resonance lines
- III / Interstellar Absorption and Emission
- A. Absorption Lines
- 1. Observations of interstellar Lyman-? absorption
- 2. Observations of interstellar Lyman-? with the Orbiting Astronomical Observatory
- 3. Interstellar lines other than hydrogen
- 4. Interstellarmolecular hydrogen (Abstract)
- 5. General discussion
- B. Emission
- 1. The night sky brightness measured from satellites Kosmos 51 and 213
- 2. Mariner 5 measurements of ultraviolet emission from the Galaxy
- 3. The ultraviolet background (intergalactic gas, the Galaxy, and subcosmic rays)
- 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 Å to 6500 Å
- 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