CMG2010 G329.337+0.147

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0.04 UTI
0.0
CN
0.08
Cdens
0.12
CC3
0.0
Clit
1.0
Cdup
N50 (P>50% members) 16
Stellar density (N50/rad) 0.4 [N/pc2]
C3 classification DC
  • CN 0.0 Sparse
  • Cdens 0.08 Very loose
  • CC3 0.12 Very low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique
đŸ“Ĩ Members 📊 Colab đŸ”Ŧ Bayestar19 MOCAMOCA 🔍 CDS 🔍 Simbad 🔍 CDS (Îą, δ) 🔍 Simbad (Îą, δ)

Overview
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CMG2010 G329.337+0.147 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a moderate* distance, near the mid-plane. It is catalogued as a very young cluster (see Parameters). It is rarely studied in the literature, with no articles listed in the last 13 years.

(*): The parallax distance estimate (~2.60 kpc) differs significantly from the median photometric distance (~7.08 kpc).

⚠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.

Morales et al. (2013)
Classified as morphological type 'EC1' (deeply embedded cluster). Morphological flag: cluster fully embedded.

Data
🔍 Search references for CMG2010 G329.337+0.147 in: SciX Simbad
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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 240.187 -52.726 0.385 -4.74 -4.882 -29.996
Morales et al. 2013 240.138 -52.746 – – – –

💡 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– 7.08 – – 1 – – – –
Morales et al. 2013 7.08 – – 1 – – – –

Visualization
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CMG2010 G329.337+0.147 UCC
Galactocentric position diagram