NGC 110
(OCL 300; MWSC 45)
Summary
NGC 110 is a sparse, very loose object of low C3 quality. It is located at a large 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.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| Dias et al. (2002) | 6.854 | 71.383 | – | 0.01 | -3.47 | – |
| Kharchenko et al. (2012) | 6.855 | 71.422 | – | 2.75 | 3.78 | – |
| Loktin & Popova (2017) | 6.855 | 71.383 | – | 3.308 | 3.589 | – |
| Bica et al. (2019) | 6.836 | 71.381 | – | – | – | – |
| UCC | 6.957 | 71.357 | 0.182 | -1.553 | -0.22 | -74.225 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Dias et al. (2002) | E(B-V)=0.42, Dist=1290.0, Age=9.0 |
| Kharchenko et al. (2012) | e_bv=0.65, distance=1600, log_age=8.97 |
| Loktin & Popova (2017) | E(B-V)=0.252, Dist=1872, logt=9.35 |
Search coordinates in Bayestar19