CWWDL 2577

0.05 UTI

0.3

C_N

0.54

C_dens

0.38

C_C3

0.0

C_lit

0.2

C_dup

C3 classification CB

Number of members (P>50%) 30

Radius (P>50% members) 3.4 [arcmin]

C_N 0.3 Poorly populated
C_dens 0.54 Moderately dense
C_C3 0.38 Low quality
C_lit 0.0 Rarely studied
C_dup 0.2 Likely duplicate

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

Overview

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CWWDL 2577 is a poorly populated, moderately dense object of low C3 quality. Its parallax locates it at a moderate 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 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 Very young

Data

🔍 Search references for CWWDL 2577 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	–	345.5	60.357	0.296	-4.007	-2.543	-70.674
Chi et al.	2023	345.531	60.326	0.303	-3.956	-2.542	–

💡 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	–	–	–	0	0.320	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CWNU 1774	80.0	345.47	60.36	0.3	-4.01	-2.54	-70.67	0.3

💡 Note: The % column shows the percentage of members that CWWDL 2577 shares with each listed object.

Visualization

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