IRAS 00013+6817
Summary
IRAS 00013+6817 is a sparse, very loose object of very low C3 quality. It is located at a large distance from the Sun, well 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 |
|---|---|---|---|---|---|---|
| Kharchenko et al. (2012) | 0.996 | 68.565 | – | -3.52 | -1.55 | – |
| UCC | 0.756 | 68.55 | 0.168 | -1.655 | -0.501 | -97.8 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Kharchenko et al. (2012) | e_bv=0.833, distance=1338, log_age=7.15 |
Search coordinates in Bayestar19