Latham 1
(MWSC 2084)
Summary
Latham 1 is a sparse, very loose object of very low C3 quality. It is located at a close distance from the Sun, well 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.
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 |
|---|---|---|---|---|---|---|
| Dias et al. (2002) | 197.708 | 30.477 | – | -2.32 | -3.2 | -2.4 |
| Kharchenko et al. (2012) | 197.812 | 30.525 | – | -7.3 | -1.37 | – |
| Bica et al. (2019) | 197.71 | 30.477 | – | – | – | – |
| UCC | 197.902 | 30.588 | 1.452 | 4.472 | -10.246 | 38.885 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Dias et al. (2002) | E(B-V)=0.208, Dist=1015.0, Age=9.4 |
| Kharchenko et al. (2012) | e_bv=0.208, distance=1015, log_age=9.4 |
Search coordinates in Bayestar19