FSR 1755
0.18
UTI
0.39
CN
0.38
Cdens
0.12
CC3
0.0
Clit
1.0
Cdup
Stellar density (N50/rad)
1.9 [N/pc2]
- CN 0.39 Poorly populated
- Cdens 0.38 Loose
- CC3 0.12 Very low quality
- Clit 0.0 Rarely studied
- Cdup 1.0 Unique
đĨ Members
đ Colab
đŦ Bayestar19
MOCA
đ CDS
đ Simbad
đ CDS (Îą, δ)
đ Simbad (Îą, δ)
MOCA
đ CDS
đ Simbad
đ CDS (Îą, δ)
đ Simbad (Îą, δ)
Overview
FSR 1755 is a poorly populated, loose object of very low C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane. No fundamental parameter values are available for this object. It is rarely studied in the literature, with no articles listed in the last 12 years.
Note: This object shares a significant percentage of members with 3 later reported entries. 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.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 258.095 | -38.445 | 0.612 | -2.633 | -3.643 | -36.133 |
| Dias et al. | 2014 | 258.083 | -38.462 | â | -2.63 | -3.6 | â |
| Froebrich et al. | 2007 | 258.083 | -38.462 | â | â | â | â |
| Dias et al. | 2002 | 258.083 | -38.462 | â | -2.63 | -3.6 | â |
đĄ Note: The UCC values are estimated from its identified members.
