NGC 7175
(MWSC 3577)
Summary
NGC 7175 is a sparse, very loose object of very low C3 quality. It is located at a large distance from the Sun, near 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) | 329.692 | 54.818 | – | -2.86 | -4.36 | -26.82 |
| Kharchenko et al. (2012) | 329.767 | 54.79 | – | -3.73 | -1.31 | – |
| Bica et al. (2019) | 329.701 | 54.816 | – | – | – | – |
| UCC | 329.74 | 54.788 | 0.146 | -2.548 | -2.155 | -86.672 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Dias et al. (2002) | E(B-V)=0.87, Dist=1930.0, Age=8.4 |
| Kharchenko et al. (2012) | e_bv=0.75, distance=2500, log_age=8.821 |
Search coordinates in Bayestar19