CWWDL 14595

0.10 UTI

0.38

C_N

0.53

C_dens

1.0

C_C3

0.0

C_lit

0.26

C_dup

C3 classification AA

Number of members (P>50%) 38

Radius (P>50% members) 35.6 [arcmin]

C_N 0.38 Poorly populated
C_dens 0.53 Moderately dense
C_C3 1.0 Very high quality
C_lit 0.0 Rarely studied
C_dup 0.26 Possibly duplicate

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

Overview

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CWWDL 14595 is a poorly populated, moderately 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 14595 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	–	122.358	-46.771	2.733	-6.229	9.014	16.279
Chi et al.	2023	122.416	-46.643	2.705	-6.226	8.989	0.457

💡 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	–	–	–	2	-0.100	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
OCSN 254	73.7	122.38	-47.34	2.89	-6.4	9.6	14.61	0.07
Pozzo 1	65.8	122.39	-47.33	2.89	-6.41	9.61	15.22	1.0
CWWDL 14592	23.7	123.01	-46.3	2.79	-6.35	9.19	15.12	0.16
CWWDL 14586	18.4	121.61	-48.0	2.74	-6.0	9.04	18.68	0.26

💡 Note: The % column shows the percentage of members that CWWDL 14595 shares with each listed object.

Visualization

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