CWWDL 1627

0.35 UTI

0.88

C_N

1.0

C_dens

1.0

C_C3

0.0

C_lit

0.61

C_dup

C3 classification AA

Number of members (P>50%) 444

Radius (P>50% members) 8.3 [arcmin]

C_N 0.88 Rich
C_dens 1.0 Very dense
C_C3 1.0 Very high quality
C_lit 0.0 Rarely studied
C_dup 0.61 Likely unique

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

Overview

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CWWDL 1627 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 metal-poor, very young cluster (see Parameters). It was recently reported in the literature.

Note: This is likely a unique object, which shares a moderate percentage of members with at least one previously reported entry. See table with shared members information.

Metal-poor Very young

Data

🔍 Search references for CWWDL 1627 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	–	263.986	-33.963	0.388	-0.144	-1.494	15.772
Chi et al.	2023	263.958	-33.984	0.385	-0.078	-1.528	4.602

💡 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	-0.580	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 565	39.0	264.03	-33.91	0.39	-0.16	-1.47	-10.15	0.73

💡 Note: The % column shows the percentage of members that CWWDL 1627 shares with each listed object.

Visualization

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