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Modeling Eclipses of the Novalike Variable TT Triangulum
2006
Publications of the Astronomical Society of the Pacific
Multicolor (BVRI) light curves of the eclipsing novalike variable TT Tri are presented and analyzed with a parameter-fitting eclipse model. The mass ratio of TT Tri is poorly constrained, but must lie roughly in the range 0.3>R_1) generally resulted in a higher white dwarf temperature, and a steepening of the disk temperature profile, but were not required to achieve a viable steady-state disk solution. No evidence was found for a luminous bright spot in the system, which is not surprising
doi:10.1086/508555
fatcat:dqjmpypepzduxfhlzw3xxaflmq