CWNU 1654

0.20 UTI

0.0

C_N

0.13

C_dens

0.25

C_C3

0.3

C_lit

1.0

C_dup

N₅₀ (P>50% members) 19

Stellar density (N₅₀/rad) 0.6 [N/pc²]

C3 classification CC

C_N 0.0 Sparse
C_dens 0.13 Very loose
C_C3 0.25 Low quality
C_lit 0.3 Poorly studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

ℹ️

CWNU 1654 is a sparse, very loose object of low C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane, affected by low extinction. It is catalogued as a low-mass, near-solar metallicity, young cluster (see Parameters). It was recently reported in the literature.

Relatively close Low extinction Low mass Near-solar metallicity Young

Cavallo et al. (2024)
Gold sample.

Data

🔍 Search references for CWNU 1654 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	99999–	89.642	16.182	0.728	1.173	-2.23	15.625
Zhang et al.	2024	89.629	16.208	–	–	–	–
Hunt & Reffert	2024	89.629	16.208	0.726	1.151	-2.184	15.623
Cavallo et al.	2024	89.643	16.192	0.723	–	–	–
Hunt & Reffert	2023	89.629	16.208	0.726	1.151	-2.184	15.623
He et al.	2023	89.633	16.19	0.732	1.17	-2.243	–

💡 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–	1.37	0.87	0.79	65	-0.161	42	–	–
Zhang et al.	2024	–	–	–	–	-0.251⁽¹⁾	–	–	–
Hunt & Reffert	2024	–	–	–	–	–	42⁽¹⁾	–	–
Cavallo et al.	2024	1.37	0.87	–	65	-0.070	–	–	–
Hunt & Reffert	2023	1.34	0.63	0.79	194	–	–	–	–
He et al.	2023	1.41	1.05	–	40	–	–	–	–

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

Visualization

ℹ️

1 2