Dias 8
(MWSC 3195)
Summary
Dias 8 is a sparse, very loose object of very low C3 quality. It is located at a moderate distance from the Sun, 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.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| Dias et al. (2002) | 298.025 | 11.634 | – | -2.56 | -3.28 | – |
| Kharchenko et al. (2012) | 298.043 | 11.628 | – | -1.22 | -3.07 | – |
| Loktin & Popova (2017) | 298.035 | 11.628 | – | -1.054 | -3.214 | – |
| Bica et al. (2019) | 298.035 | 11.634 | – | – | – | – |
| UCC | 298.011 | 11.611 | 0.291 | -4.83 | -6.338 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Dias et al. (2002) | E(B-V)=0.3, Dist=2220.0, Age=9.35 |
| Kharchenko et al. (2012) | e_bv=0.312, distance=4785, log_age=9.15 |
| Loktin & Popova (2017) | E(B-V)=0.062, Dist=2246, logt=9.8 |
Search coordinates in Bayestar19