CWWDL 245

0.02 UTI

0.37

C_N

1.0

C_dens

0.5

C_C3

0.0

C_lit

0.05

C_dup

C3 classification BB

Number of members (P>50%) 37

Radius (P>50% members) 2.5 [arcmin]

C_N 0.37 Poorly populated
C_dens 1.0 Very dense
C_C3 0.5 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 0.05 Very likely duplicate

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

Overview

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CWWDL 245 is a poorly populated, very dense object of intermediate C3 quality. Its parallax locates it at a moderate distance, below the mid-plane. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It was recently reported in the literature.

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

Near-solar metallicity Young

Data

🔍 Search references for CWWDL 245 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	–	94.473	9.68	0.305	-1.022	-0.048	43.727
Chi et al.	2023	94.468	9.694	0.3	-0.986	-0.023	36.079

💡 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	–	–	–	25	0.440	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CWNU 1550	94.6	94.47	9.68	0.3	-1.01	-0.05	43.73	0.38
Theia 4212	89.2	94.47	9.68	0.3	-1.01	-0.07	43.73	0.04

💡 Note: The % column shows the percentage of members that CWWDL 245 shares with each listed object.

Visualization

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