CWWDL 14597

0.31 UTI

0.42

C_N

0.38

C_dens

0.75

C_C3

0.0

C_lit

1.0

C_dup

C3 classification AB

Number of members (P>50%) 42

Radius (P>50% members) 28.8 [arcmin]

C_N 0.42 Poorly populated
C_dens 0.38 Loose
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 1.0 Unique

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

Overview

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CWWDL 14597 is a poorly populated, loose object of high C3 quality. Its parallax locates it at a 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 object shares a large percentage of members 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 14597 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	–	157.744	-64.281	1.786	-16.852	1.808	-4.275
Chi et al.	2023	157.541	-64.47	1.798	-16.884	1.854	-4.457

💡 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	–	–	–	6	-0.280	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 2384	90.5	158.56	-64.22	1.8	-16.85	1.61	-4.12	0.06
CWWDL 14602	88.1	158.5	-64.2	1.8	-16.85	1.67	-4.47	0.45

💡 Note: The % column shows the percentage of members that CWWDL 14597 shares with each listed object.

Visualization

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