NGC 2413
(MWSC 1262)
Summary
NGC 2413 is a sparse, very loose object of very low C3 quality. It is located at a moderate distance from the Sun, above 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) | 113.279 | -13.4 | – | -2.35 | 2.13 | – |
| Piskunov et al. (2008) | 113.275 | -13.036 | – | – | – | – |
| Kharchenko et al. (2012) | 113.265 | -12.99 | – | -0.47 | 1.61 | – |
| Loktin & Popova (2017) | 113.28 | -13.399 | – | 0.773 | -0.162 | – |
| Bica et al. (2019) | 113.31 | -13.097 | – | – | – | – |
| UCC | 113.331 | -13.112 | 0.277 | -1.371 | 0.484 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Dias et al. (2002) | E(B-V)=0.04, Dist=440.0, Age=8.46 |
| Piskunov et al. (2008) | E(B-V)=0.04, Dist=440, logt=8.46, logMA=1.296 |
| Kharchenko et al. (2012) | e_bv=0.042, distance=1341, log_age=8.655 |
| Loktin & Popova (2017) | E(B-V)=0.149, Dist=763, logt=8.576 |
Search coordinates in Bayestar19