NGC 2352
(ESO 492 05; MWSC 1143)
Summary
NGC 2352 is a sparse, very loose object of low C3 quality. It is located at a large distance from the Sun, 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) | 108.271 | -24.038 | – | -2.13 | 4.3 | – |
| Kharchenko et al. (2012) | 108.272 | -24.029 | – | -3.34 | 6.75 | – |
| Loktin & Popova (2017) | 108.27 | -24.029 | – | -4.011 | 4.591 | – |
| Bica et al. (2019) | 108.277 | -24.042 | – | – | – | – |
| UCC | 108.339 | -24.037 | 0.196 | -1.192 | 2.232 | 58.726 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Dias et al. (2002) | E(B-V)=0.32, Dist=1750.0, Age=8.08 |
| Kharchenko et al. (2012) | e_bv=0.666, distance=3000, log_age=8.775 |
| Loktin & Popova (2017) | E(B-V)=0.597, Dist=8325, logt=7.66 |
Search coordinates in Bayestar19