Ultraviolet photometry and spectrophotometry of Algol

Details Ultraviolet photometry and spectrophotometry of Algol Ultraviolet photometry and spectrophotometry of Algol

Oct 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975pasp...87..745e&link_type=abstract

Astronomical Society of the Pacific, Publications, vol. 87, Oct. 1975, p. 745-751.

Astronomy and Astrophysics

Astrophysics

16

Astronomical Photometry, Eclipsing Binary Stars, Light Curve, Stellar Spectrophotometry, Stellar Temperature, Ultraviolet Radiation, Algol, Energy Spectra, Oao 2, Radiant Flux Density, Tables (Data)

Scientific paper

OAO-2 blue and UV light curves and spectrophotometric observations are used to establish effective temperatures and luminosities for the three components of the eclipsing Algol (beta Persei) system. An essentially complete energy distribution is given for Algol, and the fundamental properties - geometrical quantities, wavelength-dependent quantities and derived astrophysical quantities - are presented for the star.

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