Astronomy and Astrophysics – Astrophysics
Scientific paper
Oct 1997
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997nasa.repty....s&link_type=abstract
Technical Report, NASA/CR-97-205745; NAS 1.26:205745 Advanced Technology Center
Astronomy and Astrophysics
Astrophysics
Eclipsing Binary Stars, High Temperature Plasmas, Abundance, Iron, Light Curve, Extreme Ultraviolet Explorer Satellite, Polynomials, X Ray Spectra, Cosmology, X Ray Timing Explorer
Scientific paper
EUVE, Advanced Satellite for Cosmology and Astrophysics (ASCA), and X-ray Timing Explorer (XTE) observed the eclipsing binary Algol (Beta Per) from 1-7 Feb 1996. The coordinated observation covered approx. 2 binary orbits of the system, with a net exposure of approx. 160 ksec for EUVE, 40 ksec for ASCA (in 4 pointings), and 90 ksec for XTE (in 45 pointings). We discuss results of modeling the combined EUVE, ASCA, and XTE data using continuous differential emission measure distributions, and provide constraints on the abundance in the Algol system.
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