NGC 2579
0.30
UTI
0.32
CN
0.28
Cdens
0.25
CC3
0.31
Clit
1.0
Cdup
Radius (P>50% members)
2.7 [arcmin]
- CN 0.32 Poorly populated
- Cdens 0.28 Loose
- CC3 0.25 Low quality
- Clit 0.31 Poorly studied
- Cdup 1.0 Unique
Overview
NGC 2579 is a poorly populated, loose object of low C3 quality. Its parallax locates it at a large* distance, near the mid-plane, affected by low extinction. It is catalogued as a young cluster (see Parameters). It is poorly studied in the literature, with no articles listed in the last 9 years.
(*): The parallax distance estimate (~6.04 kpc) differs significantly from the median photometric distance (~1.03 kpc).
Note: This object shares a significant percentage of members with a later reported entry. See table with shared members information.
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.
Relatively close
Low extinction
Young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 125.223 | -36.217 | 0.166 | -2.443 | 3.046 | â |
| Loktin & Popova | 2017 | 125.22 | -36.217 | â | -3.39 | 0.64 | 1.6 |
| Dias et al. | 2014 | 125.217 | -36.217 | â | -3.93 | 0.64 | â |
| Gozha et al. | 2012 | 125.217 | -36.217 | â | â | â | â |
| van den Bergh | 2006 | 125.221 | -36.213 | â | â | â | â |
| Dias et al. | 2002 | 125.217 | -36.217 | â | -3.93 | 0.64 | 1.65 |
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 |
|---|---|---|---|---|---|---|---|---|---|
| Loktin & Popova | 2017 | 0.89 | 0.42 | â | 56 | â | â | â | â |
| Gozha et al. | 2012 | 1.03 | â | â | 41 | â | â | â | â |
| van den Bergh | 2006 | 1.03 | 0.46 | â | 41 | â | â | â | â |
| Dias et al. | 2002 | 1.03 | 0.46 | â | 41 | â | â | â | â |
