IRAS 17301 2917
Summary
IRAS 17301 2917 is a sparse, very loose object of low C3 quality. It is located at a large distance from the Sun, 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 |
|---|---|---|---|---|---|---|
| Dias et al. (2002) | 263.342 | -29.178 | – | 0.66 | 0.77 | – |
| Kharchenko et al. (2012) | 263.332 | -29.165 | – | 0.66 | 0.77 | – |
| UCC | 263.318 | -29.145 | 0.13 | -2.985 | -1.627 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Dias et al. (2002) | E(B-V)=2.415, Dist=1215.0, Age=7.2 |
| Kharchenko et al. (2012) | e_bv=2.415, distance=1215, log_age=7.2 |
Search coordinates in Bayestar19