NGC 6604

(MWSC 2878)

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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

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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.

Almeida et al. (2025)
Mass determination: intermediate fit. Isochrone match: intermediate fit.

Cavallo et al. (2024)
Silver sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 274.485 -12.213 0.47 -0.435 -2.396 -9.308
Almeida et al. 2025 274.513 -12.245 – – – –
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 – – –
Hunt & Reffert 2023 274.526 -12.253 0.459 -0.447 -2.45 -49.566
Almeida et al. 2023 274.525 -12.243 – – – –
Just et al. 2023 274.5 -12.239 – – – –
Jaehnig et al. 2021 274.476 -12.124 0.494 -0.4 -2.181 –
Dias et al. 2021 274.513 -12.245 0.454 -0.453 -2.294 –
Loktin & Popova 2017 274.515 -12.243 – 1.537 -7.304 9.6
Kharchenko et al. 2016 274.5 -12.239 – – – –
Dias et al. 2014 274.512 -12.242 – -2.15 -3.05 –
Kharchenko et al. 2013 274.507 -12.238 – -0.22 -2.7 9.6
Gozha et al. 2012 274.512 -12.242 – – – –
Piskunov et al. 2008 274.505 -12.245 – – – –
Kharchenko et al. 2007 274.51 -12.24 – 0.26 – 9.6
Piskunov et al. 2007 274.505 -12.245 – – – –
van den Bergh 2006 274.5 -12.233 – – – –
Kharchenko et al. 2005 274.51 -12.24 – -0.36 -2.68 9.6
Kharchenko et al. 2003 274.53 -12.23 – -0.45 -2.57 –
Chen et al. 2003 274.534 -12.192 – -0.02 -2.74 18.0
Dias et al. 2002 274.512 -12.242 – -2.15 -3.05 -5.43
Dambis 1999 274.512 -12.242 – – – –

💡 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 99999– 1.795 2.94 0.62 6 0.104 871 0.74 –
Almeida et al. 2025 1.89 2.80 – 6 – 466 – –
Hunt & Reffert 2024 – – – – – 387(1) – –
Cavallo et al. 2024 2.09 2.58 – 43 1.070 – – –
Hunt & Reffert 2023 2.18 3.17 0.62 3 – – – –
Almeida et al. 2023 1.94 2.88 – 6 0.103 871(1) 0.74 –
Just et al. 2023 – – – 8 – 912 – –
Jaehnig et al. 2021 2.02(1) – – – – – – –
Dias et al. 2021 1.89 2.80 – 6 0.104 – – –
Loktin & Popova 2017 1.65 3.00 – 7 – – – –
Kharchenko et al. 2016 1.90 3.00 – 8 – – – –
Kharchenko et al. 2013 1.90 3.00 – 8 – – – –
Gozha et al. 2012 1.70 – – 6 – 4467 – –
Piskunov et al. 2008 1.70 2.94 – 4 – 2312(1) – –
Piskunov et al. 2007 1.70 2.94 – 4 – 364 – –
van den Bergh 2006 1.70 3.01 – 6 – – – –
Kharchenko et al. 2005 1.70 2.94 – 4 – – – –
Kharchenko et al. 2003 1.70 2.79 – – – – – –
Chen et al. 2003 1.70 – – 0 – – – –
Dias et al. 2002 1.70 3.01 – 6 – – – –
Dambis 1999 2.40 3.11 – 3 – – – –

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Cluster % RA DEC Plx pmRA pmDE Rv UTI
UBC 344 20.2 274.46 -12.08 0.47 -0.29 -2.2 55.54 0.42

💡 Note: The % column shows the percentage of members that NGC 6604 shares with each listed object.

Visualization

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