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- W3100064765 abstract "We report estimates of the masses of the component stars in the pre-main-sequence spectroscopic binary UZ Tau E. These results come from the combination of our measurements of the mass ratio, M2/M1 = 0.28 ± 0.01, obtained using high-resolution H-band spectroscopy, with the total mass of the system, (1.31 ± 0.08)(D/140 pc) M☉, derived from millimeter observations of the circumbinary disk (Simon, Dutrey, & Guilloteau). The masses of the primary and secondary are (1.016 ± 0.065)(D/140 pc) M☉ and (0.294 ± 0.027)(D/140 pc) M☉, respectively. Using the orbital parameters determined from our six epochs of observation, we find that the inclination of the binary orbit, 598 ± 44, is consistent with that determined for the circumbinary disk from the millimeter observations, indicating that the disk and binary orbits are probably coplanar." @default.
- W3100064765 created "2020-11-23" @default.
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- W3100064765 date "2002-11-10" @default.
- W3100064765 modified "2023-09-27" @default.
- W3100064765 title "Component Masses of the Young Spectroscopic Binary UZ Tau E" @default.
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- W3100064765 doi "https://doi.org/10.1086/345317" @default.
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