CWWDL 1597

0.10 UTI

0.76

C_N

1.0

C_dens

1.0

C_C3

0.0

C_lit

0.17

C_dup

C3 classification AA

Number of members (P>50%) 115

Radius (P>50% members) 3.5 [arcmin]

C_N 0.76 Rich
C_dens 1.0 Very dense
C_C3 1.0 Very high quality
C_lit 0.0 Rarely studied
C_dup 0.17 Likely duplicate

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

Overview

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CWWDL 1597 is a rich, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It was recently reported in the literature.

⚠️ Warning: This is likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.

Near-solar metallicity Young

Data

🔍 Search references for CWWDL 1597 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	–	251.82	-46.666	0.41	-1.798	-4.054	-19.988
Chi et al.	2023	251.825	-46.654	0.415	-1.774	-3.945	-22.212

💡 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	–	–	–	58	0.300	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
LISC 1757	82.6	251.81	-46.67	0.41	-1.8	-4.06	-20.0	0.11
UBC 669	67.0	251.8	-46.67	0.4	-1.8	-4.1	-19.97	0.66

💡 Note: The % column shows the percentage of members that CWWDL 1597 shares with each listed object.

Visualization

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