FSR 1518
(MWSC 1738)
0.28
UTI
0.0
CN
0.26
Cdens
0.38
CC3
0.38
Clit
1.0
Cdup
Radius (P>50% members)
2.2 [arcmin]
- CN 0.0 Sparse
- Cdens 0.26 Loose
- CC3 0.38 Low quality
- Clit 0.38 Poorly studied
- Cdup 1.0 Unique
Overview
FSR 1518 is a sparse, loose object of low C3 quality. Its parallax locates it at a large* distance, above the mid-plane, affected by moderate extinction. It is catalogued as a young cluster (see Parameters). It is poorly studied in the literature.
(*): The parallax distance estimate (~6.63 kpc) differs significantly from the median photometric distance (~1.82 kpc).
Note: This object shares a significant percentage of members with a later reported entry. See table with shared members information.
â ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.
Relatively close
Moderate extinction
Young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 149.845 | -54.513 | 0.151 | -4.542 | 2.578 | 57.334 |
| Just et al. | 2023 | 149.874 | -54.506 | â | â | â | â |
| Kharchenko et al. | 2016 | 149.874 | -54.506 | â | â | â | â |
| Dias et al. | 2014 | 149.871 | -54.518 | â | -6.82 | -0.19 | â |
| Kharchenko et al. | 2013 | 149.88 | -54.51 | â | -4.09 | 2.38 | â |
| Froebrich et al. | 2007 | 149.871 | -54.518 | â | â | â | â |
| Dias et al. | 2002 | 149.871 | -54.518 | â | -4.09 | 2.38 | â |
đĄ Note: The UCC values are estimated from its identified members.
| Reference | Year | Dist [kpc] | Av [mag] | DAv [mag] | Age [Myr] | [Fe/H] [dex] | Mass [Msun] | Bfr | BSS |
|---|---|---|---|---|---|---|---|---|---|
| Just et al. | 2023 | â | â | â | 40 | â | 97 | â | â |
| Kharchenko et al. | 2016 | 1.82 | 1.94 | â | 40 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.82 | 1.94 | â | 40 | â | â | â | â |
| Dias et al. | 2002 | 1.82 | 1.94 | â | 40 | â | â | â | â |
