NGC 2180
(MWSC 765)
Summary
NGC 2180 is a sparse, very loose object of low C3 quality. It is located at a moderate 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 |
|---|---|---|---|---|---|---|
| Piskunov et al. (2008) | 92.436 | 4.81 | – | – | – | – |
| Kharchenko et al. (2012) | 92.438 | 4.805 | – | 0.6 | 0.19 | – |
| Loktin & Popova (2017) | 92.445 | 4.807 | – | 0.039 | -0.495 | – |
| Angelo et al. (2019) | 92.433 | 4.823 | – | – | – | – |
| Bica et al. (2019) | 92.45 | 4.806 | – | – | – | – |
| UCC | 92.454 | 4.788 | 0.202 | 0.156 | 0.2 | 48.648 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Piskunov et al. (2008) | E(B-V)=0.0, Dist=910, logt=9.24, logMA=1.937 |
| Kharchenko et al. (2012) | e_bv=0.396, distance=1882, log_age=9.355 |
| Loktin & Popova (2017) | E(B-V)=0.291, Dist=1962, logt=8.1 |
| Angelo et al. (2019) | dsun=1.05, Age=0.71, Mphot=27 |
Search coordinates in Bayestar19