CWWDL 5091

0.04 UTI

0.58

C_N

1.0

C_dens

0.75

C_C3

0.0

C_lit

0.09

C_dup

C3 classification AB

Number of members (P>50%) 66

Radius (P>50% members) 3.7 [arcmin]

C_N 0.58 Moderately populated
C_dens 1.0 Very dense
C_C3 0.75 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

ℹ️

CWWDL 5091 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a moderate 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 5091 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	159.026	-60.634	0.407	-7.694	2.637	-7.446
Chi et al.	2023	159.002	-60.635	0.42	-7.62	2.671	–

💡 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	0.270	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Theia 3409	95.5	159.03	-60.65	0.4	-7.72	2.65	-7.45	0.03
UBC 1483	90.9	159.03	-60.64	0.41	-7.72	2.65	-7.45	0.5

💡 Note: The % column shows the percentage of members that CWWDL 5091 shares with each listed object.

Visualization

ℹ️