CWWDL 2647

0.07 UTI

0.54

C_N

0.78

C_dens

0.75

C_C3

0.0

C_lit

0.16

C_dup

C3 classification AB

Number of members (P>50%) 57

Radius (P>50% members) 3.3 [arcmin]

C_N 0.54 Moderately populated
C_dens 0.78 Dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.16 Likely duplicate

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

Overview

ℹ️

CWWDL 2647 is a moderately populated, dense object of high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It was recently reported in the literature.

⚠️ Warning: This is 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 Young

Data

🔍 Search references for CWWDL 2647 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	90.564	26.147	0.251	0.182	-1.027	48.367
Chi et al.	2023	90.553	26.111	0.267	0.177	-1.206	41.296

💡 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	–	–	–	87	0.120	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Teutsch 92	84.2	90.56	26.15	0.24	0.15	-0.98	19.35	0.65
UBC 1301	66.7	90.56	26.15	0.27	0.14	-0.98	14.97	0.01

💡 Note: The % column shows the percentage of members that CWWDL 2647 shares with each listed object.

Visualization

ℹ️