ESO 427 32
Summary
ESO 427 32 is a sparse, very loose object of low C3 quality. It is located at a large distance from the Sun, well below the mid-plane. It is poorly studied in the literature, with no articles listed in the last 8 years.
Warning: contains less than 25 stars with P>0.5 estimated.
Warning: the low UTI value and no obvious signs of duplication (C_dup=1.0) indicates that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| Dias et al. (2002) | 106.558 | -30.167 | – | 0.98 | 1.98 | – |
| Kharchenko et al. (2012) | 106.582 | -30.16 | – | 0.18 | 2.55 | – |
| Loktin & Popova (2017) | 106.53 | -30.18 | – | 0.219 | 2.514 | – |
| UCC | 106.622 | -30.169 | 0.129 | -1.141 | 1.66 | 38.835 |
Estimated members
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Fundamental parameters
| Reference | Values |
|---|---|
| Dias et al. (2002) | E(B-V)=0.125, Dist=1786.0, Age=9.105 |
| Kharchenko et al. (2012) | e_bv=0.125, distance=1786, log_age=9.105 |
| Loktin & Popova (2017) | E(B-V)=0.115, Dist=2315, logt=9.18 |
Search coordinates in Bayestar19