CWWDL 14577

0.00 UTI

0.3

C_N

0.58

C_dens

1.0

C_C3

0.0

C_lit

0.0

C_dup

C3 classification AA

Number of members (P>50%) 30

Radius (P>50% members) 28.4 [arcmin]

C_N 0.3 Poorly populated
C_dens 0.58 Moderately dense
C_C3 1.0 Very high quality
C_lit 0.0 Rarely studied
C_dup 0.0 Very likely duplicate

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

Overview

ℹ️

CWWDL 14577 is a poorly populated, moderately dense object of very high C3 quality. Its parallax locates it at a very close distance, below 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 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 Very young

Data

🔍 Search references for CWWDL 14577 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	104.14	-26.703	2.573	-6.112	6.045	20.678
Chi et al.	2023	104.11	-26.652	2.577	-6.146	5.997	25.271

💡 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	–	–	–	4	0.400	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CWNU 1024	100.0	104.4	-26.87	2.51	-6.02	6.02	21.44	0.56
OCSN 144	100.0	104.27	-26.59	2.52	-6.01	6.01	21.57	0.07

💡 Note: The % column shows the percentage of members that CWWDL 14577 shares with each listed object.

Visualization

ℹ️