NGC 6895
(MWSC 3296)
Summary
NGC 6895 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 rarely 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 |
|---|---|---|---|---|---|---|
| Kharchenko et al. (2012) | 304.035 | 50.245 | – | -3.42 | -2.34 | – |
| Bica et al. (2019) | 304.103 | 50.23 | – | – | – | – |
| UCC | 304.077 | 50.231 | 0.335 | -4.155 | -5.617 | -68.76 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Kharchenko et al. (2012) | e_bv=0.208, distance=1935, log_age=9.33 |
Search coordinates in Bayestar19