Comparison between theoretical colors calculated from model atmospheres and ultraviolet celescope observations of supergiant star atmospheres show that most stars are deficient in ultraviolet flux relative to theoretical models. It is concluded that not enough line blocking has been included in model atmospheres
The properties of the chromospheres, transition regions and coronas of cool evolved stars are review...
The discrepancy between observed and calculated ultraviolet fluxes of A to G stars can be largely al...
IUE observations of the late-type M supergiant TV Gem (M1 lab) have been obtained that reveal strong...
Data from Project Celescope, a program that photographed the ultraviolet sky, in order to study seve...
We undertake an optical and ultraviolet spectroscopic analysis of a sample of 20 Galactic B0-B5 supe...
A survey of F supergiant stars to evaluate the extension of chromospheric and circumstellar characte...
Data obtained from approximately 7500 ultraviolet television pictures are used to compile a celescop...
The accumulation of photoelectric data on the Johnson-Morgan system of B - V and U - B colors makes ...
The spectra for B stars for which emission lines occur not on the main sequence, but only among the ...
Aims. We undertake an optical and ultraviolet spectroscopic analysis of a sample of 20 Galactic B0-B...
Scans of lambda Lep, eta UMa, xi Dra, epsilon Dor, alpha Leo, phi Dra, upsilon Dra, beta Aur, alpha ...
Color indices for stellar spectrophotometry of Cepheid variable and supergiant star
Broad band filter photometry for 57 bright stars of spectral type A2 discussed with peak instrument ...
Filter photometry has been used to derive the interstellar reddening law from stars through the stud...
The filter photometers in the Wisconsin Experiment Package on OAO-2 were used to obtain data for a c...
The properties of the chromospheres, transition regions and coronas of cool evolved stars are review...
The discrepancy between observed and calculated ultraviolet fluxes of A to G stars can be largely al...
IUE observations of the late-type M supergiant TV Gem (M1 lab) have been obtained that reveal strong...
Data from Project Celescope, a program that photographed the ultraviolet sky, in order to study seve...
We undertake an optical and ultraviolet spectroscopic analysis of a sample of 20 Galactic B0-B5 supe...
A survey of F supergiant stars to evaluate the extension of chromospheric and circumstellar characte...
Data obtained from approximately 7500 ultraviolet television pictures are used to compile a celescop...
The accumulation of photoelectric data on the Johnson-Morgan system of B - V and U - B colors makes ...
The spectra for B stars for which emission lines occur not on the main sequence, but only among the ...
Aims. We undertake an optical and ultraviolet spectroscopic analysis of a sample of 20 Galactic B0-B...
Scans of lambda Lep, eta UMa, xi Dra, epsilon Dor, alpha Leo, phi Dra, upsilon Dra, beta Aur, alpha ...
Color indices for stellar spectrophotometry of Cepheid variable and supergiant star
Broad band filter photometry for 57 bright stars of spectral type A2 discussed with peak instrument ...
Filter photometry has been used to derive the interstellar reddening law from stars through the stud...
The filter photometers in the Wisconsin Experiment Package on OAO-2 were used to obtain data for a c...
The properties of the chromospheres, transition regions and coronas of cool evolved stars are review...
The discrepancy between observed and calculated ultraviolet fluxes of A to G stars can be largely al...
IUE observations of the late-type M supergiant TV Gem (M1 lab) have been obtained that reveal strong...
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