CWWDL 14102

0.19 UTI

0.52

C_N

0.55

C_dens

0.75

C_C3

0.0

C_lit

0.53

C_dup

C3 classification AB

Number of members (P>50%) 53

Radius (P>50% members) 10.6 [arcmin]

C_N 0.52 Moderately populated
C_dens 0.55 Moderately dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.53 Likely unique

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

Overview

ℹ️

CWWDL 14102 is a moderately populated, moderately dense object of high C3 quality. Its parallax locates it at a relatively 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.

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.

Near-solar metallicity Very young

Data

🔍 Search references for CWWDL 14102 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	124.421	-43.62	0.7	-4.968	4.448	28.897
Chi et al.	2023	124.405	-43.647	0.705	-4.916	4.436	29.275

💡 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	–	–	–	12	0.440	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 1584	47.2	124.4	-43.6	0.71	-4.98	4.44	41.35	0.5
CWNU 12	43.4	124.46	-43.62	0.71	-5.0	4.45	31.11	0.08

💡 Note: The % column shows the percentage of members that CWWDL 14102 shares with each listed object.

Visualization

ℹ️