CWWDL 14592

0.16 UTI

0.42

C_N

1.0

C_dens

1.0

C_C3

0.0

C_lit

0.33

C_dup

C3 classification AA

Number of members (P>50%) 42

Radius (P>50% members) 21.3 [arcmin]

C_N 0.42 Poorly populated
C_dens 1.0 Very dense
C_C3 1.0 Very high quality
C_lit 0.0 Rarely studied
C_dup 0.33 Possibly duplicate

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

Overview

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CWWDL 14592 is a poorly populated, very 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.

⚠️ Warning: This is possibly a duplicate object, which shares a significant percentage of members with at least one previously reported entry, and a 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 14592 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	–	123.01	-46.303	2.793	-6.352	9.186	15.125
Chi et al.	2023	122.864	-46.28	2.769	-6.374	9.186	2.67

💡 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	–	–	–	1	-0.100	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
OCSN 254	66.7	122.38	-47.34	2.89	-6.4	9.6	14.61	0.07
Pozzo 1	59.5	122.39	-47.33	2.89	-6.41	9.61	15.22	1.0
CWWDL 14595	21.4	122.36	-46.77	2.73	-6.23	9.01	16.28	0.1
CWWDL 14593	19.0	123.1	-46.18	2.87	-6.51	9.41	15.29	0.11

💡 Note: The % column shows the percentage of members that CWWDL 14592 shares with each listed object.

Visualization

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