Loden 1095
(OCL 913.1; MWSC 2174)
Summary
Loden 1095 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.
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) | 208.375 | -59.75 | – | -3.74 | -4.85 | – |
| Kharchenko et al. (2012) | 208.403 | -59.745 | – | -9.64 | -2.12 | – |
| Bica et al. (2019) | 208.244 | -59.658 | – | – | – | – |
| UCC | 208.262 | -59.686 | 0.321 | -7.284 | -1.446 | -8.728 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Dias et al. (2002) | E(B-V)=0.854, Dist=4028.0, Age=8.55 |
| Kharchenko et al. (2012) | e_bv=0.854, distance=4028, log_age=8.55 |
Search coordinates in Bayestar19