CWWDL 14586

0.26 UTI

0.62

C_N

0.53

C_dens

1.0

C_C3

0.0

C_lit

0.61

C_dup

C3 classification AA

Number of members (P>50%) 74

Radius (P>50% members) 49.9 [arcmin]

C_N 0.62 Moderately populated
C_dens 0.53 Moderately 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

ℹ️

CWWDL 14586 is a moderately populated, moderately dense object of very high C3 quality. Its parallax locates it at a very close distance, near 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, and a very small percentage with at least one entry reported in the same catalogue. See table with shared members information.

Near-solar metallicity Very young

Data

🔍 Search references for CWWDL 14586 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	121.615	-47.998	2.737	-5.995	9.044	18.675
Chi et al.	2023	121.06	-48.458	2.762	-5.987	9.03	4.93

💡 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	–	–	–	1	-0.100	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
OCSN 254	39.2	122.38	-47.34	2.89	-6.4	9.6	14.61	0.07
Pozzo 1	31.1	122.39	-47.33	2.89	-6.41	9.61	15.22	1.0
CWWDL 14595	9.5	122.36	-46.77	2.73	-6.23	9.01	16.28	0.1

💡 Note: The % column shows the percentage of members that CWWDL 14586 shares with each listed object.

Visualization

ℹ️