CWWDL 1757

0.05 UTI

0.76

C_N

1.0

C_dens

1.0

C_C3

0.0

C_lit

0.09

C_dup

C3 classification AA

Number of members (P>50%) 120

Radius (P>50% members) 3.2 [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 0.09 Very likely duplicate

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

Overview

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CWWDL 1757 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 very 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 1757 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	–	281.916	-3.816	0.457	-0.646	-1.878	9.484
Chi et al.	2023	281.912	-3.807	0.467	-0.63	-1.907	12.017

💡 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	–	–	–	66	0.440	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 355	90.8	281.92	-3.82	0.46	-0.65	-1.87	9.48	0.73
OC 0053	34.2	281.92	-3.81	0.47	-0.7	-1.87	4.3	0.0

💡 Note: The % column shows the percentage of members that CWWDL 1757 shares with each listed object.

Visualization

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