NGC 6846
(MWSC 3207)
0.78
UTI
0.76
CN
1.0
Cdens
0.75
CC3
0.7
Clit
1.0
Cdup
Radius (P>50% members)
0.9 [arcmin]
- CN 0.76 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.7 Moderately studied
- Cdup 1.0 Unique
Overview
NGC 6846 is a rich, very dense object of high C3 quality. Its parallax locates it at a very large* distance, above the mid-plane, affected by high extinction. It is catalogued as a massive, metal-poor, intermediate-age cluster (see Parameters). It is moderately studied in the literature.
(*): The parallax distance estimate (~12.41 kpc) differs significantly from the median photometric distance (~5.32 kpc).
Very distant
High extinction
Massive
Metal-poor
Intermediate age
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 299.117 | 32.351 | 0.081 | -2.884 | -5.054 | -43.175 |
| Hunt & Reffert | 2024 | 299.115 | 32.35 | 0.088 | -2.873 | -5.097 | -42.508 |
| Cavallo et al. | 2024 | 299.101 | 32.337 | 0.09 | â | â | â |
| Hunt & Reffert | 2023 | 299.115 | 32.35 | 0.088 | -2.873 | -5.097 | -42.508 |
| Just et al. | 2023 | 299.103 | 32.352 | â | â | â | â |
| Cantat-Gaudin et al. | 2020 | 299.112 | 32.349 | 0.089 | -2.971 | -4.994 | â |
| Cantat-Gaudin & Anders | 2020 | 299.112 | 32.349 | 0.089 | -2.971 | -4.994 | â |
| Soubiran et al. | 2018 | 299.112 | 32.349 | â | â | â | -42.94 |
| Cantat-Gaudin et al. | 2018 | 299.112 | 32.349 | 0.089 | -2.971 | -4.994 | â |
| Kharchenko et al. | 2016 | 299.103 | 32.352 | â | â | â | â |
| Dias et al. | 2014 | 299.117 | 32.348 | â | -0.05 | -1.36 | â |
| Kharchenko et al. | 2013 | 299.109 | 32.355 | â | 0.12 | -3.95 | â |
| Dias et al. | 2002 | 299.117 | 32.348 | â | 0.12 | -3.95 | 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 | 2214* | â | â |
| Cavallo et al. | 2024 | 4.51 | 3.92 | â | 178 | -0.960 | â | â | â |
| Hunt & Reffert | 2023 | 9.14 | 4.18 | 2.39 | 44 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 1429 | â | 873 | â | â |
| Cantat-Gaudin et al. | 2020 | 5.32 | 2.85 | â | 490 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 8.50 | â | â | â | â | â | â | â |
| Soubiran et al. | 2018 | 8.50 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 8.50 | â | â | â | â | â | â | â |
| Kharchenko et al. | 2016 | 4.45 | 3.25 | â | 1429 | â | â | â | â |
| Kharchenko et al. | 2013 | 4.45 | 3.25 | â | 1429 | â | â | â | â |
| Dias et al. | 2002 | 4.45 | 3.26 | â | 501 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Cavallo et al. (2024)
Silver sample.