G3CC 62

0.25 UTI

0.6

C_N

0.0

C_dens

0.62

C_C3

0.0

C_lit

1.0

C_dup

N₅₀ (P>50% members) 70

Stellar density (N₅₀/rad) 0.0 [N/pc²]

C3 classification AC

C_N 0.6 Moderately populated
C_dens 0.0 Very loose
C_C3 0.62 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19

MOCA 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

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G3CC 62 is a moderately populated, very loose object of intermediate C3 quality. Its parallax locates it at a very large^* distance, well below the mid-plane. It is catalogued as a cluster (see Parameters). It is rarely studied in the literature, with no articles listed in the last 13 years.

(*): The parallax distance estimate (~91.74 kpc) differs significantly from the median photometric distance (~3.63 kpc).

Distant

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

Data

🔍 Search references for G3CC 62 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–	286.817	5.397	0.011	-2.452	-6.194	59.359
Morales et al.	2013	286.75	5.385	–	–	–	–

💡 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]	B_frac	BSS
UCC	99999–	3.63	–	–	–	–	–	–	–
Morales et al.	2013	3.63	–	–	–	–	–	–	–

Visualization

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