CWWDL 14622

0.35 UTI

0.36

C_N

0.86

C_dens

1.0

C_C3

0.0

C_lit

0.78

C_dup

C3 classification AA

Number of members (P>50%) 36

Radius (P>50% members) 22.4 [arcmin]

C_N 0.36 Poorly populated
C_dens 0.86 Dense
C_C3 1.0 Very high quality
C_lit 0.0 Rarely studied
C_dup 0.78 Very likely unique

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

Overview

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CWWDL 14622 is a poorly populated, dense object of very high C3 quality. Its parallax locates it at a very close 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.

Note: This is very likely a unique object, which shares a small 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 14622 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	–	345.679	58.217	2.25	5.425	-1.308	-8.928
Chi et al.	2023	345.524	58.234	2.263	5.31	-1.289	-41.638

💡 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	–	–	–	7	0.070	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
RSG8	22.2	345.42	59.37	2.07	5.59	-1.67	-7.68	0.87
RSG7	19.4	343.99	59.45	2.35	4.94	-1.81	-12.62	0.37

💡 Note: The % column shows the percentage of members that CWWDL 14622 shares with each listed object.

Visualization

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