NGC 7127
Summary
NGC 7127 is a sparse, very loose object of low C3 quality. It is located at a large distance from the Sun, above 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) | 325.921 | 54.63 | – | -4.05 | -3.92 | – |
| Kharchenko et al. (2012) | 325.921 | 54.615 | – | -7.47 | -1.99 | – |
| UCC | 325.841 | 54.6 | 0.163 | -2.272 | -2.102 | -63.09 |
Estimated members
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Fundamental parameters
| Reference | Values |
|---|---|
| Dias et al. (2002) | E(B-V)=0.9, Dist=1445.0, Age=8.6 |
| Kharchenko et al. (2012) | e_bv=1.031, distance=2300, log_age=8.8 |
Search coordinates in Bayestar19