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Table 2
Relative positions of the Mira binary system.
Epoch | Δαcosδ | Δδ | ρ | θ | Telescope | Reference |
′′ | ′′ | ′′ | ° | |||
|
||||||
1995.9467 | 0.549 ± 0.002 | −0.182 ± 0.002 | 0.578 | 108.3 | HST | Karovska et al. (1997) |
2004.1295 | 0.525 ± 0.003 | −0.149 ± 0.003 | 0.546 | 105.8 | HST | Ireland et al. (2007) |
2004.1342 | 0.5281 ± 0.0008 | −0.1465 ± 0.0008 | 0.5480 | 105.51 | HST | This paper |
2007.7283 | 0.5093 ± 0.0020 | −0.1258 ± 0.0022 | 0.5246 | 103.87 | HST | This paper |
2014.1478 | 0.4721 ± 0.0006 | −0.0792 ± 0.0007 | 0.4787 | 99.53 | JVLA | Matthews, priv. comm. |
2014.4517 | 0.4687 ± 0.0006 | −0.0750 ± 0.0005 | 0.4747 | 99.09 | ALMA band 7 | This paper |
2014.4572 | 0.4695 ± 0.0003 | −0.0752 ± 0.0003 | 0.4755 | 99.10 | ALMA band 9 | This paper |
2014.8050 | 0.46620 ± 0.00011 | −0.07119 ± 0.00010 | 0.47161 | 98.68 | ALMA band 3 | This paper |
2014.8309 | 0.46610 ± 0.00007 | −0.06980 ± 0.00008 | 0.47129 | 98.52 | ALMA band 6 | This paper |
Notes. ρ is the star separation and θ is the position angle. The uncertainties in the offsets are the formal errors in the Gaussian fits.
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