NGC 1520
Summary
NGC 1520 is a sparse, very loose object of high C3 quality. It is located at a very large distance from the Sun, well below the mid-plane. It is poorly studied in the literature, with no articles listed in the last 8 years.
Warning: contains less than 25 stars with P>0.5 estimated.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| Dias et al. (2002) | 59.462 | -76.795 | – | 4.39 | 3.83 | – |
| Kharchenko et al. (2012) | 59.468 | -76.8 | – | 4.96 | -3.37 | – |
| Loktin & Popova (2017) | 59.46 | -76.794 | – | 3.575 | 5.339 | – |
| UCC | 59.521 | -76.762 | 0.041 | 1.793 | -0.437 | – |
Estimated members
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Fundamental parameters
| Reference | Values |
|---|---|
| Dias et al. (2002) | E(B-V)=0.06, Dist=775.0, Age=9.3 |
| Kharchenko et al. (2012) | e_bv=0.0, distance=1023, log_age=9.43 |
| Loktin & Popova (2017) | E(B-V)=0.208, Dist=1089, logt=9.56 |
Search coordinates in Bayestar19