CWWDL 14587

0.17 UTI

0.0

C_N

0.37

C_dens

0.75

C_C3

0.0

C_lit

0.76

C_dup

C3 classification AB

Number of members (P>50%) 21

Radius (P>50% members) 29.6 [arcmin]

C_N 0.0 Sparse
C_dens 0.37 Loose
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.76 Very likely unique

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

Overview

ℹ️

CWWDL 14587 is a sparse, loose object of 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 very likely a unique object, which shares a small percentage of members with at least one previously reported entry. See table with shared members information.

⚠️ Warning: the low UTI value and no obvious signs of duplication (C_dup=0.76) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Near-solar metallicity Very young

Data

🔍 Search references for CWWDL 14587 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	122.071	-49.849	2.565	-5.399	8.331	17.422
Chi et al.	2023	122.501	-49.83	2.58	-5.43	8.335	22.191

💡 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	0.300	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
OCSN 199	24.0	119.78	-49.16	2.47	-5.39	8.25	20.01	0.43

💡 Note: The % column shows the percentage of members that CWWDL 14587 shares with each listed object.

Visualization

ℹ️