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| 01546+2049 | MKT 3 | bet Ari = Sheratan. Astrometry from Mark III interferometer is combined | |
| | MKT 3 | with spectroscopy (Tomkin & Tran 1987) by Pan et al. (1990) to | Tom1987b |
| | MKT 3 | determine orbital elements, masses, and distance. Masses agree well | MkT1990 |
| | MKT 3 | with empirical mass-luminosity relation. | |
| | MKT 3 | Hipparcos astrometric solution adopted some elements from the orbit of | HIP1997d |
| | MKT 3 | Pan et al. (1990). | MkT1990 |
| | MKT 3 | Martin et al. (1998) derive component masses 2.067 ± 0.203 and | |
| | MKT 3 | 1.281 ± 0.178 Msun. | Mig1998 |
| | MKT 3 | Pourbaix gives combined solution for this resolved SB2, yielding | |
| | MKT 3 | orbital parallaxes and component masses. | Pbx2000b |
| | MKT 3 | Malkov et al. (2012) derive dynamical, photometric, and spectroscopic | |
| | MKT 3 | masses of 3.19 ± 0.13, 3.51, and 1.82 Msun, respectively. | Mlk2012 |
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