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Дата изменения: Mon Jan 14 18:42:41 2002 Дата индексирования: Mon Oct 1 22:19:41 2012 Кодировка: koi8-r Поисковые слова: m 11 |
Stellar magnitudes, provided by observations in an optical band,
are reduced to the units of erg/cm/s as follows:
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(4.1) |
The -value is corrected by us according to the paper by
Bochkarev et al (1991), where disk color indexes are calculated
with a certain distribution of the temperature along the radius
and the real shapes of transmission bands of optical filters
are taken into account.
We have achieved coincidence between theoretical values by
Bochkarev et al (1991) and ours, obtained with rectangular shapes
of transmission band of optical filters.
For the effect, it was enough to correct the value of `zero-point' for B band.
Refs:
Бочкарев и др. (Bochkarev N.G., Karitskaya E.A., Shakura N.I., Zhekov S.A.) // Astron. Astrophys. Trans., 1991, V. 1, P. 41.
Zombeck M.V. // Handbook of Astronomy and Astrophysics, 1990, Cambridge, UK. http://adsbit.harvard.edu/books/hsaa/index.html