Results 121 to 130 of about 334 (164)
Addendum - Detection of Mass Loss in Stellar Chromospheres
The Astrophysical Journal, 1980 R. E. Stencel, D. J. Mullan
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Evidence for stellar chromospheres presented by ultraviolet observations of the sun and stars
, 1973 L. R. Doherty
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Heating of Stellar Chromospheres by Shock Waves.
The Astrophysical Journal, 1960 openaire +1 more source
PREDICTED ULTRAVIOLET SPECTRA FROM STELLAR CHROMOSPHERES
Journal of Quantitative Spectroscopy and Radiative Transfer, 1968 Abstract Perhaps the most tangible evidence of the existence and structure of postulated stellar chromospheres of otherwise relatively cool stars would be the detection of an intense ultraviolet spectrum. The solar case for which a variety of measurements is available now reveals that the observed spectrum depends in a very complex and not thoroughly
Ludwig Oster, N. P. Patterson
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A phenomenological interpretation of stellar chromospheres
Astrophysics and Space Science, 1986 An attempt is made to develop a phenomenological interpretation of stellar chromospheres. The following problems are examined: observed emission powers of ‘magnesium’ chromospheres on stars based on the ultraviolet doublet, 2800 Mgii, observations; dependence of chromosphere emission on spectral and luminosity classes; stellar chromospheres as an ...
G. A. Gurzadyan
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Solar and stellar chromospheric contrast
Solar Physics, 1994We present an analysis of disk-integrated spectra of the Caii K line (3933.68 A). The selection of parameters in the line profile, and the correlations between them, follow the work of Smith (1960), but represent an innovative aspect in the fact that our data are spatially integrated.
Robert A. Donahue +2 more
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