NGC 6604
(MWSC 2878)
0.95
UTI
0.76
CN
1.0
Cdens
1.0
CC3
1.0
Clit
1.0
Cdup
Stellar density (N50/rad)
13.5 [N/pc2]
- CN 0.76 Rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
NGC 6604 is a rich, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, very young cluster, but with a large variance across recent sources for the age and metallicity parameters (see Parameters). It is very well-studied in the literature.
Note: This object shares a small percentage of members with a later reported entry. See table with shared members information.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 274.485 | -12.213 | 0.47 | -0.435 | -2.396 | -9.308 |
| Almeida et al. | 2025 | 274.513 | -12.245 | â | â | â | â |
| Hunt & Reffert | 2024 | 274.526 | -12.253 | 0.459 | -0.447 | -2.45 | -49.566 |
| Cavallo et al. | 2024 | 274.52 | -12.246 | 0.461 | â | â | â |
| Hunt & Reffert | 2023 | 274.526 | -12.253 | 0.459 | -0.447 | -2.45 | -49.566 |
| Almeida et al. | 2023 | 274.525 | -12.243 | â | â | â | â |
| Just et al. | 2023 | 274.5 | -12.239 | â | â | â | â |
| Jaehnig et al. | 2021 | 274.476 | -12.124 | 0.494 | -0.4 | -2.181 | â |
| Dias et al. | 2021 | 274.513 | -12.245 | 0.454 | -0.453 | -2.294 | â |
| Loktin & Popova | 2017 | 274.515 | -12.243 | â | 1.537 | -7.304 | 9.6 |
| Kharchenko et al. | 2016 | 274.5 | -12.239 | â | â | â | â |
| Dias et al. | 2014 | 274.512 | -12.242 | â | -2.15 | -3.05 | â |
| Kharchenko et al. | 2013 | 274.507 | -12.238 | â | -0.22 | -2.7 | 9.6 |
| Gozha et al. | 2012 | 274.512 | -12.242 | â | â | â | â |
| Piskunov et al. | 2008 | 274.505 | -12.245 | â | â | â | â |
| Kharchenko et al. | 2007 | 274.51 | -12.24 | â | 0.26 | â | 9.6 |
| Piskunov et al. | 2007 | 274.505 | -12.245 | â | â | â | â |
| van den Bergh | 2006 | 274.5 | -12.233 | â | â | â | â |
| Kharchenko et al. | 2005 | 274.51 | -12.24 | â | -0.36 | -2.68 | 9.6 |
| Kharchenko et al. | 2003 | 274.53 | -12.23 | â | -0.45 | -2.57 | â |
| Chen et al. | 2003 | 274.534 | -12.192 | â | -0.02 | -2.74 | 18.0 |
| Dias et al. | 2002 | 274.512 | -12.242 | â | -2.15 | -3.05 | -5.43 |
| Dambis | 1999 | 274.512 | -12.242 | â | â | â | 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] | Bfrac | BSS |
|---|---|---|---|---|---|---|---|---|---|
| UCC | 99999â | 1.795 | 2.94 | 0.62 | 6 | 0.104 | 871 | 0.74 | â |
| Almeida et al. | 2025 | 1.89 | 2.80 | â | 6 | â | 466 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 387(1) | â | â |
| Cavallo et al. | 2024 | 2.09 | 2.58 | â | 43 | 1.070 | â | â | â |
| Hunt & Reffert | 2023 | 2.18 | 3.17 | 0.62 | 3 | â | â | â | â |
| Almeida et al. | 2023 | 1.94 | 2.88 | â | 6 | 0.103 | 871(1) | 0.74 | â |
| Just et al. | 2023 | â | â | â | 8 | â | 912 | â | â |
| Jaehnig et al. | 2021 | 2.02(1) | â | â | â | â | â | â | â |
| Dias et al. | 2021 | 1.89 | 2.80 | â | 6 | 0.104 | â | â | â |
| Loktin & Popova | 2017 | 1.65 | 3.00 | â | 7 | â | â | â | â |
| Kharchenko et al. | 2016 | 1.90 | 3.00 | â | 8 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.90 | 3.00 | â | 8 | â | â | â | â |
| Gozha et al. | 2012 | 1.70 | â | â | 6 | â | 4467 | â | â |
| Piskunov et al. | 2008 | 1.70 | 2.94 | â | 4 | â | 2312(1) | â | â |
| Piskunov et al. | 2007 | 1.70 | 2.94 | â | 4 | â | 364 | â | â |
| van den Bergh | 2006 | 1.70 | 3.01 | â | 6 | â | â | â | â |
| Kharchenko et al. | 2005 | 1.70 | 2.94 | â | 4 | â | â | â | â |
| Kharchenko et al. | 2003 | 1.70 | 2.79 | â | â | â | â | â | â |
| Chen et al. | 2003 | 1.70 | â | â | 0 | â | â | â | â |
| Dias et al. | 2002 | 1.70 | 3.01 | â | 6 | â | â | â | â |
| Dambis | 1999 | 2.40 | 3.11 | â | 3 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Almeida et al. (2025)
Mass determination: intermediate fit. Isochrone match: intermediate fit.
Cavallo et al. (2024)
Silver sample.