NGC 2132
(ESO 120 22; MWSC 694)
Summary
NGC 2132 is a sparse, very loose object of high C3 quality. It is located at a very large distance from the Sun, well below the mid-plane. It is poorly studied in the literature, with no articles listed in the last 6 years.
Warning: contains less than 25 stars with P>0.5 estimated.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| Dias et al. (2002) | 88.787 | -59.91 | – | 1.14 | 5.52 | – |
| Kharchenko et al. (2012) | 88.83 | -59.92 | – | -1.33 | 7.43 | – |
| Loktin & Popova (2017) | 88.83 | -59.91 | – | 0.703 | 2.696 | – |
| Bica et al. (2019) | 88.848 | -59.908 | – | – | – | – |
| UCC | 88.743 | -59.869 | -0.009 | 1.748 | 0.612 | 291.459 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Dias et al. (2002) | E(B-V)=0.06, Dist=974.0, Age=9.22 |
| Kharchenko et al. (2012) | e_bv=0.291, distance=1003, log_age=9.045 |
| Loktin & Popova (2017) | E(B-V)=0.106, Dist=1755, logt=9.2 |
Search coordinates in Bayestar19