NGC 2579

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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

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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.

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.

Relatively close Low extinction Young

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 125.223 -36.217 0.166 -2.443 3.046 –
Loktin & Popova 2017 125.22 -36.217 – -3.39 0.64 1.6
Dias et al. 2014 125.217 -36.217 – -3.93 0.64 –
Gozha et al. 2012 125.217 -36.217 – – – –
van den Bergh 2006 125.221 -36.213 – – – –
Dias et al. 2002 125.217 -36.217 – -3.93 0.64 1.65

💡 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 – 56 – – – –
Gozha et al. 2012 1.03 – – 41 – – – –
van den Bergh 2006 1.03 0.46 – 41 – – – –
Dias et al. 2002 1.03 0.46 – 41 – – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 4164 75.0 125.22 -36.22 0.16 -2.43 3.01 – 0.01

💡 Note: The % column shows the percentage of members that NGC 2579 shares with each listed object.

Visualization

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