QUASISYNTHETIC PHOTOMETRY

Автор(и)

  • V. Tsymbal Tavrian National University Vernadskiy's Avenue 4, Simferopol, Crimea, 95007, Ukraine; Institut fur Astronomie Universitat Wien, Turkenschanzstrasse 17, 1180 Wien, Austria, Україна

DOI:

https://doi.org/10.18524/1810-4215.2008.21.86878

Ключові слова:

Stars, absolute spectrophotometry, angular diameters, individual, Vega, Procyon.

Анотація

The brief description of new ideas for the flux calibration of stellar spectra are presented. Described approach lets us to produce a lot of reference stars both for ground and space observations. The metodology also opens possibilities to determine the angular diameters from high resolution stellar spectra and analyze the interstellar medium in the direction of a star.

Посилання

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Hayes D.: 1985, Calibration of F undamental Stellar Quantities, Proc. of IAU Symposium No.111, /ed. D.S.Hayes, L.E.Pasinetti, A.G.Davis Phillip (Reidel, Dordre cht), 225.

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Komarov N., Karamysh V., Dragunova A., et.al.: 1979, Photometric and spectral catalogue of the bright stars: Kyiv, Naukova dumka.

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Опубліковано

2008-12-20

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