C1331 622
(MWSC 2137)
Summary
C1331 622 is a sparse, very loose object of low C3 quality. It is located at a large distance from the Sun, near the mid-plane. It is poorly studied in the literature.
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) | 203.55 | -62.417 | – | -1.59 | -4.43 | -35.0 |
| Kharchenko et al. (2013) | 203.655 | -62.417 | – | -7.61 | 0.93 | – |
| Kharchenko et al. (2016) | 203.644 | -62.414 | – | – | – | – |
| Just et al. (2023) | 203.644 | -62.414 | – | – | – | – |
| UCC | 203.611 | -62.353 | 0.175 | -6.959 | -1.269 | -22.097 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Dias et al. (2002) | E(B-V)=0.23, Dist=819.0 |
| Kharchenko et al. (2013) | E(B-V)=0.271, d=1078.0, logt=9.25 |
| Kharchenko et al. (2016) | E(B-V)=0.271, d=1078.0, logt=9.25 |
| Just et al. (2023) | logt=9.25, logmt=1.54 |
Search coordinates in Bayestar19