Astronomy and Astrophysics – Astronomy
Scientific paper
Nov 1984
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984mnras.211..229b&link_type=abstract
Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 211, Nov. 1, 1984, p. 229-234.
Astronomy and Astrophysics
Astronomy
8
B Stars, Eclipsing Binary Stars, Stellar Spectrophotometry, Telescopes, Light Curve, Mass Ratios, Spectrum Analysis, Stellar Magnitude, Stellar Models
Scientific paper
The refurbished twin photometric telescope at St. Andrews has been used to obtain a complete B light curve (≡1150 observations) of the B-type interacting binary system TT Aurigae. Analysis of the light curve by the synthesis code LIGHT (Hill 1979) results in an rms scatter of the individual observations about the theoretical model fit of ±0.005 mag. The system is shown to be in a semi-detached state but with too large a mass ratio to be considered as a classical Algol system.
Bell Aaron S.
Hilditch Ron W.
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