NGC 6883
(MWSC 3275)
0.74
UTI
0.38
CN
1.0
Cdens
0.75
CC3
0.79
Clit
1.0
Cdup
Radius (P>50% members)
2.8 [arcmin]
- CN 0.38 Poorly populated
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.79 Well-studied
- Cdup 1.0 Unique
Overview
NGC 6883 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a moderate* distance, above the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It is well-studied in the literature.
(*): The parallax distance estimate (~2.05 kpc) differs significantly from the median photometric distance (~1.38 kpc).
Note: This object shares a large percentage of members with a later reported entry. See table with shared members information.
Relatively close
Low extinction
Near-solar metallicity
Young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 302.849 | 35.858 | 0.489 | -3.139 | -6.245 | -24.132 |
| Hunt & Reffert | 2024 | 302.846 | 35.837 | 0.482 | -3.097 | -6.219 | -23.106 |
| Cavallo et al. | 2024 | 302.89 | 35.892 | 0.486 | â | â | â |
| Hunt & Reffert | 2023 | 302.846 | 35.837 | 0.482 | -3.097 | -6.219 | -23.106 |
| Just et al. | 2023 | 302.83 | 35.827 | â | â | â | â |
| Loktin & Popova | 2017 | 302.835 | 35.833 | â | -0.692 | -0.869 | -10.3 |
| Kharchenko et al. | 2016 | 302.83 | 35.827 | â | â | â | â |
| Dias et al. | 2014 | 302.829 | 35.832 | â | -2.1 | -4.13 | â |
| Kharchenko et al. | 2013 | 302.835 | 35.83 | â | -3.5 | -5.2 | -10.3 |
| Gozha et al. | 2012 | 302.829 | 35.832 | â | â | â | â |
| Piskunov et al. | 2008 | 302.829 | 35.822 | â | â | â | â |
| Kharchenko et al. | 2007 | 302.83 | 35.83 | â | 0.16 | â | -10.33 |
| Kharchenko et al. | 2005 | 302.83 | 35.83 | â | -3.78 | -6.58 | -10.33 |
| Kharchenko et al. | 2003 | 302.83 | 35.85 | â | -2.38 | -7.72 | â |
| Dias et al. | 2002 | 302.829 | 35.832 | â | -2.89 | -6.53 | -8.18 |
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] | Bfr | BSS |
|---|---|---|---|---|---|---|---|---|---|
| Hunt & Reffert | 2024 | â | â | â | â | â | 339* | â | â |
| Cavallo et al. | 2024 | 1.62 | 1.69 | â | 8 | -0.270 | â | â | â |
| Hunt & Reffert | 2023 | 1.97 | 1.55 | 1.34 | 8 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 51 | â | 254 | â | â |
| Loktin & Popova | 2017 | 2.91 | 1.33 | â | 1023 | â | â | â | â |
| Kharchenko et al. | 2016 | 1.38 | 0.93 | â | 51 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.38 | 0.93 | â | 51 | â | â | â | â |
| Gozha et al. | 2012 | 1.38 | â | â | â | â | 269 | â | â |
| Piskunov et al. | 2008 | 1.38 | 0.93 | â | 34 | â | â | â | â |
| Kharchenko et al. | 2005 | 1.38 | 0.93 | â | 34 | â | â | â | â |
| Kharchenko et al. | 2003 | 1.38 | 0.93 | â | â | â | â | â | â |
| Dias et al. | 2002 | 1.38 | 0.93 | â | â | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Cavallo et al. (2024)
Gold sample.