NGC 6639

(MWSC 2934; OCL 57)

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0.35 UTI
0.0
CN
0.03
Cdens
0.62
CC3
0.55
Clit
1.0
Cdup
Radius (P>50% members) 3.9 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.03 Very loose
  • CC3 0.62 Intermediate quality
  • Clit 0.55 Moderately studied
  • Cdup 1.0 Unique

Overview

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NGC 6639 is a sparse, very loose object of intermediate C3 quality. Its parallax locates it at a large* distance, below the mid-plane, affected by low extinction. It is catalogued as an intermediate-age cluster (see Parameters). It is moderately studied in the literature.

(*): The parallax distance estimate (~9.19 kpc) differs significantly from the median photometric distance (~0.70 kpc).

âš ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Close Low extinction Intermediate age

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 277.725 -13.158 0.109 -3.82 -6.875 120.635
Just et al. 2023 277.732 -13.141 – – – –
Bica et al. 2019 277.716 -13.168 – – – –
Kharchenko et al. 2016 277.732 -13.141 – – – –
Dias et al. 2014 277.746 -13.155 – -0.36 -2.87 –
Kharchenko et al. 2013 277.74 -13.14 – 1.99 -1.8 7.0
Gozha et al. 2012 277.746 -13.155 – – – –
Piskunov et al. 2008 277.734 -13.155 – – – –
Kharchenko et al. 2007 277.74 -13.15 – 0.18 – 7.0
Kharchenko et al. 2005 277.74 -13.15 – 2.31 -1.5 7.0

💡 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
Just et al. 2023 – – – 851 – 72 – –
Kharchenko et al. 2016 0.77 0.78 – 851 – – – –
Kharchenko et al. 2013 0.77 0.78 – 851 – – – –
Gozha et al. 2012 0.70 – – 724 – 62 – –
Piskunov et al. 2008 0.70 0.62 – 724 – – – –
Kharchenko et al. 2005 0.70 0.62 – 724 – – – –

Visualization

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