FSR 1535
Summary
FSR 1535 is a sparse, very loose object of low C3 quality. It is located at a large distance from the Sun, below the mid-plane. It is poorly 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) | 151.979 | -59.197 | – | -7.45 | 6.66 | – |
| Froebrich et al. (2007) | 151.979 | -59.197 | – | – | – | – |
| Kharchenko et al. (2012) | 152.002 | -59.195 | – | -7.45 | 6.66 | – |
| UCC | 151.857 | -59.209 | 0.154 | -5.785 | 3.477 | 44.517 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Dias et al. (2002) | E(B-V)=0.396, Dist=1602.0, Age=8.865 |
| Kharchenko et al. (2012) | e_bv=0.396, distance=1602, log_age=8.865 |
Search coordinates in Bayestar19