Contents
- Common properties of photometric systems
- Introduction
- Elements of theory of stellar photometry
- Magnitude and color indices
- Color excesses and Q parameters
- Wavelengths characterizing a photometric system
- Energy distribution in stellar spectra
- A short review of energy distribution studies
- Normal early-type stars
- Emission-line B-type stars
- Emission-line O-type stars
- metallic-line A-type stars
- Peculiar A and B stars of type CP-2
- Peculiar B stars of HgMn type
- Helium-weak stars
- Helium-rich and hydrogen-deficient stars
- Other early-type pecullar and variable stars
- White dwarfs
- Effects of axial rotation
- Normal G- and K-type stars
- M-type stars
- Carbon stars
- Stars with CH anomalies
- Barium stars
- S-type stars
- NS- and SN-type stars
- T Tauri-type stars
- Flare stars
- The halo population stars
- Interstellar extinction
- Extinction law in the visible and infrared
- Extinction law in the ultraviolet
- The modelling of the interstellar extinction law
- Circumstellar extinction
- Interstellar polarization
- Interstellar lines
- Diffuse interstellar bands
- The methods to determine the ratio of interstellar extinction
to color excess
- Neutral interstellar extinction
- Interstellar reddening in the solar vicinity
- Atmospheric extinction
- The atmospheric extinction law
- The light of the night sky
- The best observatory sites
- Determination of atmosperic extinction corrections
- The effect of atmospheric extinction on magnitude
- The effect of atmospheric extinction on color indices
- The variation of atmospheric extinction and its elemination
- Nikonov's method
- Relative methods to determine atmospheric extinction corrections
- The elimination of extinction for infrared observations
- Neutrality of extinction by atmospheric clouds
- Broad band photometric systems introduced before 1953
- The international photographic and photovisual system
- First photoelectric systems and the P, V system
- Stebbins and Whitford six-color system
- Kron R, I system
- The UGR system
- The UBV system
- History of the UBV system
- Critical discussion of transformation of the U-B color indices
outside the atmosphere
- Response functions of the UBV system
- Comparison of synthetic and observed color indices of the UBV system
- Synthetic interstellar extinctions and color excesses
- Synthetic reddening lines in the U-B, B-V diagram
- Pratical determination of reddening lines in the U-B, B-V diagram
- The ratio R.
- Intrinsic color indices (U-B) and (B-V) and reddening-free
quantities Q UBV
- Calibration of the U-B, B-V diagram in physical parameters
- Star clusters in the UBV system
- The zero-age main sequence in the U-B, B-V diagram
- The blanketing effect in the U-B, B-V diagram and the position of
subdwarfs, metal-deficient giants, and metallic-line stars
- The solar UBV colors and its analogs
- The effect of rapid stellar axial rotation the UBV system
- Unresolved binary stars in the U-B, B-V diagram
- Black bodies in the U-B, B-V diagram
- The U-B, B-V diagram for different types of stars
- The revision of the ultraviolet magnitude of the UBV system
- The dependence of extinction coefficients of color indices of the UBV
and WBV systems on the energy distribution
- Cape observatory UcBV system
- Broad bandpass systems containing infrared
- Tasks of the infrared photometry
- The Arizona broad-band photometric system
- The R, I photometric systems after Arizona
- The Cousins R, I System
- The Washington photometric system
- The cosmological photometric systems
- Photometry in the far infrared
- Some applications of the infrared photometry
- The uvby Beta system
- General properties
- Quantification of B-type stars
- Quantification of F-type stars
- Quantification of A-type stars
- G- and K-type stars
- Stars with different pecularities
- Spectral classification from the uvby Beta photometry
- Other uvby Beta applications
- Stability and accuracy of the uvby Beta system
- Other medium- and narrow-band photometric systems
- The Geneva system
- The DDO system
- The Walraven system
- The Borgman system and the Arizona medium-band system
- The Wing infrared system and related systems
- The ultraviolet photometric systems
- Other medium-band photometric systems
- Narrow-band photometric systems
- The Vilnius photometric system
- Introduction
- Selection of bandpasses for early-type stars
- Selection of bandpasses for late-type stars
- The final sysyem and its realization
- Reduction of color indices outside the atmosphere
- Absolute calibration of magnitudes
- Color excess ratios and Q-parameters
- Intrinsic color indices
- Classification and quantification of reddened stars of solar chemical
composition on Q, Q diagrams
- The effect of interstellar extinction law variations on the accuracy
of stellar classification
- Other methods of classification and quantification
- Determination of interstellar reddening and extinction
- F-G-K suddwarfs
- Metal-deficient giants and red horizontal branch stars
- Early-type stars with different peculiarities
- Carbon-rich stars
- Unresolved binary stars
- An outline of photometric classification
- Transformations between the Vilnius system and other systems
- The Vilgen system
- The Vilnius system applications
- Appendix
- Appendix 1. Calibration of spectral classes MK in absolute magnitudes Mv
- Appendix 2. Stellar bolometric absolute magnitudes
- Appendix 3. Logarithms of stellar effective temperature and bolometric
corrections
- Appendix 4. Logarithms of stellar surface gravities
- Appendix 5. logarithms of stellar masses
- appendix 6. Logarithms of stellar radii