NGC 5155
(MWSC 2125)
Summary
NGC 5155 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 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) | 202.47 | -63.455 | – | -7.68 | 0.2 | – |
| Bica et al. (2019) | 202.011 | -63.442 | – | – | – | – |
| UCC | 202.202 | -63.459 | 0.124 | -7.265 | -2.072 | -30.096 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Kharchenko et al. (2012) | e_bv=0.354, distance=1404, log_age=7.4 |
Search coordinates in Bayestar19