CWWDL 12760

0.17 UTI

0.55

C_N

1.0

C_dens

0.62

C_C3

0.0

C_lit

0.4

C_dup

C3 classification AC

Number of members (P>50%) 60

Radius (P>50% members) 6.7 [arcmin]

C_N 0.55 Moderately populated
C_dens 1.0 Very dense
C_C3 0.62 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 0.4 Possibly duplicate

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

Overview

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CWWDL 12760 is a moderately populated, very dense object of intermediate C3 quality. Its parallax locates it at a relatively close distance, above 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 12760 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	–	62.686	57.139	0.706	0.954	-1.085	-29.84
Chi et al.	2023	62.711	57.131	0.71	0.96	-1.123	-26.615

💡 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	–	–	–	5	0.370	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Theia 7938	95.0	62.68	57.14	0.71	0.95	-1.08	-29.84	0.02
HXHWL 73	60.0	62.69	57.14	0.71	0.98	-1.08	-29.84	0.39

💡 Note: The % column shows the percentage of members that CWWDL 12760 shares with each listed object.

Visualization

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