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Determination of the effective temperatures OF B, A, and F stars of luminosity classes III–V from the slope of the spectrum in the Balmer continuum

✍ Scribed by N. A. Sokolov

Publisher
Springer
Year
1994
Tongue
English
Weight
375 KB
Volume
37
Category
Article
ISSN
0571-7256

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A method to determine the emission measure and hence the effective extension of solar flares is described. The conditions for the Balmer continuum to be visible in disk flares is also considered. The concept of the effective mass is introduced and it is shown that this mass is a little less than tha