NGC 5299
(MWSC 2170)
Summary
NGC 5299 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 rarely studied in the literature, with no articles listed in the last 6 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 |
|---|---|---|---|---|---|---|
| Kharchenko et al. (2012) | 207.607 | -59.945 | – | -8.17 | -0.26 | – |
| Bica et al. (2019) | 207.597 | -59.93 | – | – | – | – |
| UCC | 207.481 | -59.923 | 0.294 | -7.284 | -2.71 | -49.712 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Kharchenko et al. (2012) | e_bv=0.833, distance=1847, log_age=8.7 |
Search coordinates in Bayestar19