AM 1353-265
0.06
UTI
0.25
CN
0.07
Cdens
0.0
CC3
0.0
Clit
1.0
Cdup
Nm (P>50%)
25
Core radius and density
3.5 [pc], 0.4 [pc-2]
- CN 0.25 Poorly populated
- Cdens 0.07 Very loose
- CC3 0.0 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
AM 1353-265 is a poorly populated, very loose object of very low C3 quality. Its parallax locates it at a moderate distance, well above 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 24 years.
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 | 209.065 | -27.159 | 0.425 | -9.061 | -2.083 | -17.425 |
| Dias et al. | 2002 | 209.087 | -27.167 | â | â | â | â |
đĄ Note: The UCC values are estimated from its identified members.
Dias et al. (2016)
Globular Cluster (= AM-4) (Alessi, B. S. 2005, private communication); cat V3.5 (Jan 2016)