FSR 1675
(MWSC 2358)
Summary
FSR 1675 is a sparse, very loose object of very low C3 quality. It is located at a moderate distance from the Sun, well below the mid-plane. It is poorly studied in the literature, with no articles listed in the last 6 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 |
|---|---|---|---|---|---|---|
| Froebrich et al. (2007) | 242.621 | -77.651 | – | – | – | – |
| Kharchenko et al. (2012) | 242.62 | -77.66 | – | -4.02 | -6.28 | – |
| Bica et al. (2019) | 242.6 | -77.651 | – | – | – | – |
| UCC | 242.278 | -77.619 | 0.321 | -6.606 | -5.402 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Kharchenko et al. (2012) | e_bv=0.104, distance=5666, log_age=9.2 |
Search coordinates in Bayestar19