Alessi J2327.0+55
(Alessi J2327+55; ASCC 129; MWSC 3730; Alessi 70)
0.46
UTI
0.0
CN
0.41
Cdens
0.38
CC3
0.75
Clit
1.0
Cdup
Stellar density (N50/rad)
2.1 [N/pc2]
- CN 0.0 Sparse
- Cdens 0.41 Loose
- CC3 0.38 Low quality
- Clit 0.75 Well-studied
- Cdup 1.0 Unique
Overview
Alessi J2327.0+55 is a sparse, loose object of low C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane, affected by low extinction. It is catalogued as a metal-rich, intermediate-age cluster, but with a large variance across recent sources for the age and mass parameters (see Parameters). It is well-studied in the literature.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 352.042 | 55.621 | 0.528 | -2.045 | -1.56 | -31.913 |
| Hunt & Reffert | 2024 | 352.051 | 55.615 | 0.523 | -2.031 | -1.55 | â |
| Cavallo et al. | 2024 | 352.05 | 55.634 | 0.516 | â | â | â |
| Hunt & Reffert | 2023 | 352.051 | 55.615 | 0.523 | -2.031 | -1.55 | â |
| Just et al. | 2023 | 352.02 | 55.609 | â | â | â | â |
| Bica et al. | 2019 | 351.925 | 55.588 | â | â | â | â |
| Loktin & Popova | 2017 | 351.915 | 55.592 | â | -0.062 | -0.653 | â |
| Kharchenko et al. | 2016 | 352.02 | 55.609 | â | â | â | â |
| Dias et al. | 2014 | 351.921 | 55.592 | â | -0.44 | -2.41 | â |
| Kharchenko et al. | 2013 | 352.027 | 55.613 | â | -0.63 | -2.88 | â |
| Kharchenko et al. | 2012 | 352.027 | 55.613 | â | -0.63 | -2.88 | â |
| Piskunov et al. | 2008 | 351.991 | 55.6 | â | â | â | â |
| Kharchenko et al. | 2005 | 352.0 | 55.6 | â | -1.07 | -4.12 | â |
| Dias et al. | 2002 | 351.921 | 55.592 | â | -0.44 | -2.41 | 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] | Bfrac | BSS |
|---|---|---|---|---|---|---|---|---|---|
| UCC | 99999â | 1.82 | 0.82 | 0.49 | 496 | 0.520 | 854 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 124(1) | â | â |
| Cavallo et al. | 2024 | 2.00 | 0.82 | â | 178 | 0.520 | â | â | â |
| Hunt & Reffert | 2023 | 1.82 | 0.89 | 0.49 | 165 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 1122 | â | 1585 | â | â |
| Loktin & Popova | 2017 | 1.82 | 0.16 | â | 501 | â | â | â | â |
| Kharchenko et al. | 2016 | 2.00 | 0.93 | â | 1122 | â | â | â | â |
| Kharchenko et al. | 2013 | 2.00 | 0.93 | â | 1122 | â | â | â | â |
| Kharchenko et al. | 2012 | 2.00 | 0.93 | â | 1122 | â | â | â | â |
| Piskunov et al. | 2008 | 1.00 | 0.56 | â | 490 | â | â | â | â |
| Kharchenko et al. | 2005 | 1.00 | 0.56 | â | 490 | â | â | â | â |
| Dias et al. | 2002 | 1.00 | 0.56 | â | 490 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Cavallo et al. (2024)
Gold sample.