NGC 6455
(ESO 394 03)
Summary
NGC 6455 is a sparse, very loose object of low C3 quality. It is located at a very large distance from the Sun, well below 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) | 267.938 | -35.175 | – | 1.49 | -2.77 | – |
| Bica et al. (2019) | 268.087 | -35.458 | – | – | – | – |
| UCC | 268.045 | -35.304 | 0.042 | -4.023 | -7.358 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Kharchenko et al. (2012) | e_bv=1.041, distance=2710, log_age=9.25 |
Search coordinates in Bayestar19