Application of theoretical UBVRI color-color diagrams to colorimetric analyses of various astrophysical objects

Details Application of theoretical UBVRI color-color diagrams to colorimetric analyses of various astrophysical objects Application of theoretical UBVRI color-color diagrams to colorimetric analyses of various astrophysical objects

Jul 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999arep...43..459c&link_type=abstract

Astronomy Reports, Volume 43, Issue 7, July 1999, pp.459-461

Astronomy and Astrophysics

Astronomy

6

Scientific paper

UBVRI color indices have been calculated for various kinds of radiation: blackbody radiation, radiation of hydrogen plasma that is both optically thin and optically thick in the Balmer continuum, radiation of the upper photospheres of dwarfs heated by a stationary flow of high-energy particles, synchrotron radiation, and the radiation of main-sequence stars. The results are presented in the form of four color-color diagrams: (U_B)(B_V), (U_B)(V_R), (U_B)(V_I), and (B_V)(V_R).

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