NGC 7795
Summary
NGC 7795 is a sparse, very loose object of very low C3 quality. It is located at a moderate distance from the Sun, below the mid-plane. It is rarely studied in the literature, with no articles listed in the last 13 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) | 359.654 | 60.035 | – | -0.11 | 0.82 | – |
| Kharchenko et al. (2012) | 359.409 | 60.083 | – | 1.48 | 1.71 | – |
| UCC | 359.448 | 60.049 | 0.269 | -3.09 | -1.293 | -68.063 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Dias et al. (2002) | E(B-V)=1.0, Dist=2105.0, Age=8.65 |
| Kharchenko et al. (2012) | e_bv=0.899, distance=4901, log_age=9.0 |
Search coordinates in Bayestar19