NGC 6683
(MWSC 2977; OCL 74)
0.81
UTI
0.75
CN
1.0
Cdens
1.0
CC3
0.65
Clit
1.0
Cdup
Radius (P>50% members)
3.4 [arcmin]
- CN 0.75 Rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.65 Moderately studied
- Cdup 1.0 Unique
Overview
NGC 6683 is a rich, very dense object of very high C3 quality. Its parallax locates it at a moderate* distance, near the mid-plane, affected by moderate extinction. It is catalogued as a very metal-poor, very young cluster (see Parameters). It is moderately studied in the literature.
(*): The parallax distance estimate (~3.50 kpc) differs significantly from the median photometric distance (~1.44 kpc).
Note: This object shares a very small percentage of members with a later reported entry. See table with shared members information.
Relatively close
Moderate extinction
Very metal-poor
Very young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 280.556 | -6.218 | 0.286 | -0.344 | -2.344 | 42.825 |
| Hunt & Reffert | 2024 | 280.566 | -6.225 | 0.286 | -0.343 | -2.344 | 27.792 |
| Cavallo et al. | 2024 | 280.559 | -6.227 | 0.286 | â | â | â |
| Hunt & Reffert | 2023 | 280.566 | -6.225 | 0.286 | -0.343 | -2.344 | 27.792 |
| Just et al. | 2023 | 280.547 | -6.202 | â | â | â | â |
| Bica et al. | 2019 | 280.559 | -6.208 | â | â | â | â |
| Loktin & Popova | 2017 | 280.56 | -6.208 | â | -1.542 | -3.133 | â |
| Kharchenko et al. | 2016 | 280.547 | -6.202 | â | â | â | â |
| Dias et al. | 2014 | 280.554 | -6.212 | â | -1.04 | -2.09 | â |
| Kharchenko et al. | 2013 | 280.554 | -6.2 | â | -1.32 | -4.07 | â |
| van den Bergh | 2006 | 280.55 | -6.283 | â | â | â | â |
| Dias et al. | 2002 | 280.554 | -6.212 | â | -1.04 | -2.09 | 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] | Bfr | BSS |
|---|---|---|---|---|---|---|---|---|---|
| Hunt & Reffert | 2024 | â | â | â | â | â | 1168* | â | â |
| Cavallo et al. | 2024 | 3.65 | 2.62 | â | 44 | -1.440 | â | â | â |
| Hunt & Reffert | 2023 | 3.17 | 2.10 | 1.91 | 19 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 6 | â | 76 | â | â |
| Loktin & Popova | 2017 | 1.42 | 0.26 | â | 617 | â | â | â | â |
| Kharchenko et al. | 2016 | 1.44 | 1.03 | â | 6 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.44 | 1.03 | â | 6 | â | â | â | â |
| van den Bergh | 2006 | 1.20 | 1.67 | â | 10 | â | â | â | â |
| Dias et al. | 2002 | 1.20 | 1.67 | â | 10 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Cavallo et al. (2024)
Silver sample.