Absolute monochromatic fluxes in the ultraviolet spectra of stars according to the data of Orion-2

Details Absolute monochromatic fluxes in the ultraviolet spectra of stars according to the data of Orion-2 Absolute monochromatic fluxes in the ultraviolet spectra of stars according to the data of Orion-2

Jul 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982afz....18..398g&link_type=abstract

(Astrofizika, vol. 18, July-Sept. 1982, p. 398-416) Astrophysics (ISSN 0571-7132), vol. 18, no. 3, Jan. 1983, p. 242-252. Transl

Astronomy and Astrophysics

Astronomy

1

Monochromatic Radiation, Stellar Spectra, Ultraviolet Astronomy, Astronomical Catalogs, Astronomical Photography, Spectral Energy Distribution, Ubv Spectra

Scientific paper

A method for making the transition from the relative scale of measurement of the ultraviolet spectrograms of stars photographed by means of Orion-2 to the scale of absolute energy units (erg per sq cm per sec per A) is presented. The method is then applied to a group of 30 stars in the region of Auriga, around Capella (Alpha Aur). The results are given in both tabular and graphical form. The spectral classes of the stars are in the range B2-K2, and the photovisual magnitudes range from 5.6m to 9.5m.

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