NGC 6639
(MWSC 2934; OCL 57)
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
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).
â 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
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 277.725 | -13.158 | 0.109 | -3.82 | -6.875 | 120.635 |
| Just et al. | 2023 | 277.732 | -13.141 | â | â | â | â |
| Bica et al. | 2019 | 277.716 | -13.168 | â | â | â | â |
| Kharchenko et al. | 2016 | 277.732 | -13.141 | â | â | â | â |
| Dias et al. | 2014 | 277.746 | -13.155 | â | -0.36 | -2.87 | â |
| Kharchenko et al. | 2013 | 277.74 | -13.14 | â | 1.99 | -1.8 | 7.0 |
| Gozha et al. | 2012 | 277.746 | -13.155 | â | â | â | â |
| Piskunov et al. | 2008 | 277.734 | -13.155 | â | â | â | â |
| Kharchenko et al. | 2007 | 277.74 | -13.15 | â | 0.18 | â | 7.0 |
| Kharchenko et al. | 2005 | 277.74 | -13.15 | â | 2.31 | -1.5 | 7.0 |
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 |
|---|---|---|---|---|---|---|---|---|---|
| Just et al. | 2023 | â | â | â | 851 | â | 72 | â | â |
| Kharchenko et al. | 2016 | 0.77 | 0.78 | â | 851 | â | â | â | â |
| Kharchenko et al. | 2013 | 0.77 | 0.78 | â | 851 | â | â | â | â |
| Gozha et al. | 2012 | 0.70 | â | â | 724 | â | 62 | â | â |
| Piskunov et al. | 2008 | 0.70 | 0.62 | â | 724 | â | â | â | â |
| Kharchenko et al. | 2005 | 0.70 | 0.62 | â | 724 | â | â | â | â |
