CWNU 2629

0.34 UTI

0.64

C_N

0.17

C_dens

0.75

C_C3

0.06

C_lit

1.0

C_dup

N_m (P>50%) 78

Core radius and density 3.3 [pc], 0.9 [pc^-2]

C3 classification AB

C_N 0.64 Moderately populated
C_dens 0.17 Very loose
C_C3 0.75 High quality
C_lit 0.06 Rarely studied
C_dup 1.0 Unique

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

Overview

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CWNU 2629 is a moderately populated, very loose object of high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by high extinction. It is catalogued as a massive, near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.

Relatively close High extinction Massive Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Bronze sample.

Hunt & Reffert (2024)
Classified as open cluster. CMD classes: 0.06 (50th percentile), false positive (human-assigned).

Hunt & Reffert (2023)
Classified as open cluster. CMD classes: 0.06 (50th percentile), false positive (human-assigned).

Data

🔍 Search references for CWNU 2629 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–	216.47	-59.032	0.331	-5.67	-2.65	-43.774
Hunt & Reffert	2024	216.531	-59.049	0.325	-5.658	-2.673	-47.619
Cavallo et al.	2024	216.45	-59.039	0.324	–	–	–
Hunt & Reffert	2023	216.531	-59.049	0.325	-5.658	-2.673	-47.619
He et al.	2023	216.53	-59.04	0.359	-5.645	-2.649	-10.05

💡 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–	2.69	4.315	2.89	192	0.100	1395	–	–
Hunt & Reffert	2024	2.69	4.21	2.89	244	–	1395⁽¹⁾	–	–
Cavallo et al.	2024	3.55	4.42	–	68	0.100	–	–	–
Hunt & Reffert	2023	2.69	4.21	2.89	244	–	–	–	–
He et al.	2023	2.40	4.70	–	141	–	–	–	–

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Visualization

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