NGC 6828
(MWSC 3190)
0.26
UTI
0.0
CN
0.03
Cdens
0.12
CC3
0.56
Clit
1.0
Cdup
Stellar density (N50/rad)
0.2 [N/pc2]
- CN 0.0 Sparse
- Cdens 0.03 Very loose
- CC3 0.12 Very low quality
- Clit 0.56 Moderately studied
- Cdup 1.0 Unique
Overview
NGC 6828 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a moderate* distance, well below the mid-plane, affected by low extinction. It is catalogued as a low-mass, intermediate-age cluster (see Parameters). It is moderately studied in the literature.
(*): The parallax distance estimate (~3.98 kpc) differs significantly from the median photometric distance (~0.60 kpc).
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 297.555 | 7.95 | 0.251 | -1.798 | -2.908 | -54.178 |
| Just et al. | 2023 | 297.556 | 7.903 | â | â | â | â |
| Bica et al. | 2019 | 297.561 | 7.896 | â | â | â | â |
| Loktin & Popova | 2017 | 297.54 | 7.905 | â | -2.123 | -4.756 | -21.0 |
| Kharchenko et al. | 2016 | 297.556 | 7.903 | â | â | â | â |
| Dias et al. | 2014 | 297.571 | 7.903 | â | 0.25 | -4.98 | â |
| Kharchenko et al. | 2013 | 297.562 | 7.905 | â | 0.05 | -4.35 | -21.0 |
| Gozha et al. | 2012 | 297.571 | 7.903 | â | â | â | â |
| Piskunov et al. | 2008 | 297.561 | 7.896 | â | â | â | â |
| Kharchenko et al. | 2007 | 297.57 | 7.9 | â | 0.18 | â | -21.0 |
| Kharchenko et al. | 2005 | 297.57 | 7.9 | â | -1.12 | -2.9 | -21.0 |
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 | 0.6 | 0.62 | â | 363 | â | 20 | â | â |
| Just et al. | 2023 | â | â | â | 178 | â | 15 | â | â |
| Loktin & Popova | 2017 | 2.80 | 0.67 | â | 2188 | â | â | â | â |
| Kharchenko et al. | 2016 | 0.60 | 0.52 | â | 178 | â | â | â | â |
| Kharchenko et al. | 2013 | 0.60 | 0.52 | â | 178 | â | â | â | â |
| Gozha et al. | 2012 | 0.60 | â | â | 363 | â | 26 | â | â |
| Piskunov et al. | 2008 | 0.60 | 0.62 | â | 363 | â | â | â | â |
| Kharchenko et al. | 2005 | 0.60 | 0.62 | â | 363 | â | â | â | â |
MOCA
