CWWDL 1671

0.13 UTI

0.65

C_N

1.0

C_dens

1.0

C_C3

0.0

C_lit

0.25

C_dup

C3 classification AA

Number of members (P>50%) 80

Radius (P>50% members) 3.1 [arcmin]

C_N 0.65 Moderately populated
C_dens 1.0 Very dense
C_C3 1.0 Very high quality
C_lit 0.0 Rarely studied
C_dup 0.25 Possibly duplicate

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

Overview

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CWWDL 1671 is a moderately populated, 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 possibly a duplicate object, which shares a significant 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 1671 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	–	268.11	-28.193	0.302	-0.027	-1.94	-14.584
Chi et al.	2023	268.104	-28.206	0.306	-0.091	-1.907	-34.11

💡 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	–	–	–	62	0.400	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UFMG 83	75.0	268.11	-28.19	0.3	-0.02	-1.98	-15.57	0.63
UBC 1002	68.8	268.11	-28.19	0.28	0.0	-1.96	-12.71	0.14

💡 Note: The % column shows the percentage of members that CWWDL 1671 shares with each listed object.

Visualization

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