Antalova 1
(MWSC 2605; OCL 1027.1)
0.46
UTI
0.0
CN
0.32
Cdens
0.5
CC3
0.75
Clit
1.0
Cdup
Stellar density (N50/rad)
1.6 [N/pc2]
- CN 0.0 Sparse
- Cdens 0.32 Loose
- CC3 0.5 Intermediate quality
- Clit 0.75 Well-studied
- Cdup 1.0 Unique
Overview
Antalova 1 is a sparse, loose object of intermediate C3 quality. Its parallax locates it at a relatively close* distance, above the mid-plane, affected by moderate extinction. It is catalogued as a metal-poor, intermediate-age cluster, but with a large variance across recent sources for the age parameter (see Parameters). It is well-studied in the literature.
(*): The parallax distance estimate (~1.55 kpc) differs significantly from the median photometric distance (~0.98 kpc).
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 262.216 | -31.619 | 0.646 | -0.257 | -2.74 | 24.574 |
| Hunt & Reffert | 2024 | 262.211 | -31.614 | 0.652 | -0.251 | -2.727 | â |
| Cavallo et al. | 2024 | 262.227 | -31.613 | 0.651 | â | â | â |
| Hunt & Reffert | 2023 | 262.211 | -31.614 | 0.652 | -0.251 | -2.727 | â |
| Just et al. | 2023 | 262.228 | -31.58 | â | â | â | â |
| Bica et al. | 2019 | 262.228 | -31.607 | â | â | â | â |
| Kharchenko et al. | 2016 | 262.228 | -31.58 | â | â | â | â |
| Dias et al. | 2014 | 262.225 | -31.55 | â | 0.33 | -2.89 | â |
| Kharchenko et al. | 2013 | 262.237 | -31.58 | â | -0.6 | -2.73 | -2.8 |
| Gozha et al. | 2012 | 262.225 | -31.55 | â | â | â | â |
| Piskunov et al. | 2008 | 262.218 | -31.566 | â | â | â | â |
| Kharchenko et al. | 2007 | 262.23 | -31.55 | â | 0.22 | â | 33.0 |
| Kharchenko et al. | 2005 | 262.23 | -31.57 | â | -0.24 | -3.75 | 33.0 |
| Kharchenko et al. | 2003 | 262.2 | -31.58 | â | -0.3 | -2.87 | 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 | 0.985 | 1.32 | 0.39 | 305 | -0.802 | 138 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 176(1) | â | â |
| Cavallo et al. | 2024 | 1.04 | 2.04 | â | 47 | -0.950 | â | â | â |
| Hunt & Reffert | 2023 | 1.45 | 1.76 | 0.39 | 24 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 305 | â | 116 | â | â |
| Kharchenko et al. | 2016 | 0.93 | 1.32 | â | 305 | â | â | â | â |
| Kharchenko et al. | 2013 | 0.93 | 1.32 | â | 305 | -0.655 | â | â | â |
| Gozha et al. | 2012 | 1.25 | â | â | 316 | â | 138 | â | â |
| Piskunov et al. | 2008 | 0.85 | 0.78 | â | 316 | â | â | â | â |
| Kharchenko et al. | 2005 | 0.85 | 0.78 | â | 316 | â | â | â | â |
| Kharchenko et al. | 2003 | 1.25 | 0.93 | â | â | 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.