ASCC 25
(MWSC 977)
0.26
UTI
0.0
CN
0.06
Cdens
0.12
CC3
0.56
Clit
1.0
Cdup
Stellar density (N50/rad)
0.3 [N/pc2]
- CN 0.0 Sparse
- Cdens 0.06 Very loose
- CC3 0.12 Very low quality
- Clit 0.56 Moderately studied
- Cdup 1.0 Unique
Overview
ASCC 25 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a moderate* distance, well above the mid-plane, affected by low extinction. It is catalogued as an intermediate-age cluster (see Parameters). It is moderately studied in the literature.
(*): The parallax distance estimate (~3.79 kpc) differs significantly from the median photometric distance (~1.40 kpc).
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 101.36 | 24.625 | 0.264 | -0.826 | -1.951 | 56.773 |
| Just et al. | 2023 | 101.376 | 24.597 | â | â | â | â |
| Bica et al. | 2019 | 101.385 | 24.602 | â | â | â | â |
| Kharchenko et al. | 2016 | 101.376 | 24.597 | â | â | â | â |
| Dias et al. | 2014 | 101.383 | 24.6 | â | -2.06 | -3.99 | â |
| Kharchenko et al. | 2013 | 101.385 | 24.595 | â | -0.6 | -2.66 | 21.5 |
| Gozha et al. | 2012 | 101.383 | 24.6 | â | â | â | â |
| Piskunov et al. | 2008 | 101.375 | 24.597 | â | â | â | â |
| Kharchenko et al. | 2007 | 101.38 | 24.6 | â | 0.21 | â | 21.5 |
| Kharchenko et al. | 2005 | 101.38 | 24.6 | â | 0.96 | -3.26 | 21.5 |
| Dias et al. | 2002 | 101.383 | 24.6 | â | -2.06 | -3.99 | 21.5 |
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 | 1.4 | 0.5 | â | 724 | â | 293 | â | â |
| Just et al. | 2023 | â | â | â | 1259 | â | 367 | â | â |
| Kharchenko et al. | 2016 | 1.99 | 1.03 | â | 1259 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.99 | 1.03 | â | 1259 | â | â | â | â |
| Gozha et al. | 2012 | 1.40 | â | â | 724 | â | 219 | â | â |
| Piskunov et al. | 2008 | 1.40 | 0.50 | â | 724 | â | â | â | â |
| Kharchenko et al. | 2005 | 1.40 | 0.50 | â | 724 | â | â | â | â |
| Dias et al. | 2002 | 1.40 | 0.50 | â | 724 | â | â | â | â |
MOCA
