CWWDL 2007

0.05 UTI

0.52

C_N

0.1

C_dens

1.0

C_C3

0.0

C_lit

0.15

C_dup

N_m (P>50%) 54

Core radius and density 3.9 [pc], 0.5 [pc^-2]

C3 classification AA

C_N 0.52 Moderately populated
C_dens 0.1 Very loose
C_C3 1.0 Very high quality
C_lit 0.0 Rarely studied
C_dup 0.15 Likely duplicate

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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CWWDL 2007 is a moderately populated, very loose object of very high 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 likely a duplicate object, which shares a large percentage of members with at least one previously reported entry, and a very small percentage with at least one entry reported in the same catalogue. See table with shared members information.

Near-solar metallicity Very young

Data

🔍 Search references for CWWDL 2007 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–	37.433	59.776	0.351	-0.063	-0.491	–
Chi et al.	2023	37.616	59.758	0.368	-0.078	-0.528	-33.839

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

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Ferrero 38	85.2	37.57	59.79	0.34	-0.09	-0.49	-51.17	0.33
UBC 190	83.3	37.43	59.79	0.34	-0.07	-0.49	–	0.08
OC 0249	37.0	37.37	59.83	0.35	-0.07	-0.46	–	0.03
CWWDL 8509	9.3	37.29	59.48	0.37	-0.03	-0.59	–	0.06

💡 Note: The % column shows the percentage of members that CWWDL 2007 shares with each listed object.

Visualization

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