IRAS 04324+5106
(MWSC 399)
Summary
IRAS 04324+5106 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.
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. (2013) | 69.09 | 51.18 | – | -2.45 | -4.79 | – |
| Kharchenko et al. (2016) | 69.079 | 51.179 | – | – | – | – |
| Just et al. (2023) | 69.079 | 51.179 | – | – | – | – |
| UCC | 69.05 | 51.187 | 0.429 | -0.14 | -1.354 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Kharchenko et al. (2013) | E(B-V)=1.978, d=6408.0, logt=8.38 |
| Kharchenko et al. (2016) | E(B-V)=1.978, d=6408.0, logt=8.38 |
| Just et al. (2023) | logt=8.38, logmt=3.519 |
Search coordinates in Bayestar19