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- W1989018009 abstract "This paper reports on superionized UV emission lines discovered in TT Hydrae (HD 97528), a semidetached eclipsing binary system in the Southern-Hemisphere sky. The list of emission lines observed is typical for interacting nondegenerate binaries of the Algol type, but with system-specific relative-intensity characteristics. The primary component of the system is a B9.5 V main-sequence star with effective temperature of 9800 K. Its mass equals 2.25 solar masses; the radius is 1.9 solar radii; and surface gravity log g equals 4.23. The secondary star has a mass of 0.41 solar mass and fills its critical Roche lobe. Evidence obtained on mass interaction supports the conclusion that HD 97528 is a normal semidetached system." @default.
- W1989018009 created "2016-06-24" @default.
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- W1989018009 date "1988-08-01" @default.
- W1989018009 modified "2023-09-27" @default.
- W1989018009 title "The Algol-like binary TT Hydrae - The stars, circumstellar matter, and superionized plasma" @default.
- W1989018009 doi "https://doi.org/10.1086/114845" @default.
- W1989018009 hasPublicationYear "1988" @default.
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