G 76.2-0.3

(MWSC 3336)

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0.18 UTI
0.4
CN
0.13
Cdens
0.38
CC3
0.0
Clit
1.0
Cdup
C3 classification BC
Number of members (P>50%) 40
Radius (P>50% members) 7.5 [arcmin]
  • CN 0.4 Poorly populated
  • Cdens 0.13 Very loose
  • CC3 0.38 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique
đŸ“Ĩ Members 📊 Colab đŸ”Ŧ Bayestar19 🔍 CDS 🔍 Simbad 🔍 CDS (Îą, δ) 🔍 Simbad (Îą, δ)

Overview
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G 76.2-0.3 is a poorly populated, very loose object of low C3 quality. Its parallax locates it at a moderate* distance, near the mid-plane, affected by high extinction. It is catalogued as a low-mass, young cluster (see Parameters). It is rarely studied in the literature.

(*): The parallax distance estimate (~3.59 kpc) differs significantly from the median photometric distance (~1.55 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.

Relatively close High extinction Low mass Young

Data
🔍 Search references for G 76.2-0.3 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 – 306.395 37.425 0.279 -2.974 -4.995 5.467
Just et al. 2023 306.362 37.387 – – – –
Kharchenko et al. 2016 306.362 37.387 – – – –
Kharchenko et al. 2013 306.367 37.39 – 0.0 -1.5 –

💡 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 – – – 30 – 12 – –
Kharchenko et al. 2016 1.55 4.07 – 30 – – – –
Kharchenko et al. 2013 1.55 4.07 – 30 – – – –

Visualization
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G 76.2-0.3 UCC
Galactocentric position diagram