MWSC 4288
Summary
MWSC 4288 is a sparse, very loose object of low C3 quality. It is located at a moderate distance from the Sun, well above 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 |
|---|---|---|---|---|---|---|
| Scholz et al. (2015) | 251.047 | -0.135 | – | -0.1 | -7.85 | – |
| Kharchenko et al. (2016) | 251.04 | -0.135 | – | – | – | – |
| Bica et al. (2019) | 251.048 | -0.132 | – | – | – | – |
| Just et al. (2023) | 251.04 | -0.135 | – | – | – | – |
| UCC | 251.068 | -0.098 | 0.265 | -4.119 | -5.506 | -43.128 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Scholz et al. (2015) | E(B-V)=0.781, d=1994.0, logt=9.015 |
| Kharchenko et al. (2016) | E(B-V)=0.781, d=1994.0, logt=9.015 |
| Just et al. (2023) | logt=9.015, logmt=3.377 |
Search coordinates in Bayestar19