CWWDL 1872

0.05 UTI

0.0

C_N

0.12

C_dens

0.62

C_C3

0.0

C_lit

0.36

C_dup

C3 classification CA

Number of members (P>50%) 20

Radius (P>50% members) 9.8 [arcmin]

C_N 0.0 Sparse
C_dens 0.12 Very loose
C_C3 0.62 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 0.36 Possibly duplicate

📥 Members 📊 Colab 🔬 Bayestar19 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

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CWWDL 1872 is a sparse, very loose object of intermediate C3 quality. Its parallax locates it at a moderate distance, near the mid-plane. It is catalogued as a near-solar metallicity, very young cluster (see Parameters). It was recently reported in the literature.

⚠️ Warning: This is possibly a duplicate object, which shares a significant percentage of members with at least one previously reported entry. See table with shared members information.

Near-solar metallicity Very young

Data

🔍 Search references for CWWDL 1872 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	–	305.526	37.134	0.496	-2.427	-5.33	53.948
Chi et al.	2023	305.471	37.071	0.49	-2.501	-5.335	33.383

💡 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
Chi et al.	2023	–	–	–	0	0.440	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 1101	64.0	305.72	37.19	0.49	-2.38	-5.32	46.61	0.44
Theia 1975	48.0	305.52	37.04	0.5	-2.4	-5.36	53.95	0.06
XDOCC 10	24.0	305.52	37.24	0.5	-2.4	-5.26	53.95	0.25
UBC 1098	20.0	305.39	36.93	0.49	-2.63	-5.41	-134.78	0.38

💡 Note: The % column shows the percentage of members that CWWDL 1872 shares with each listed object.

Visualization

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