CWWDL 2617

0.30 UTI

0.62

C_N

0.13

C_dens

0.75

C_C3

0.0

C_lit

0.99

C_dup

C3 classification AB

Number of members (P>50%) 74

Radius (P>50% members) 12.3 [arcmin]

C_N 0.62 Moderately populated
C_dens 0.13 Very loose
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.99 Unique

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

Overview

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CWWDL 2617 is a moderately populated, very loose 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.

Note: This is a unique object, which shares a very small percentage of members with at least one previously reported entry, and a moderate percentage with at least one entry reported in the same catalogue. See table with shared members information.

Near-solar metallicity Young

Data

🔍 Search references for CWWDL 2617 in: SciX Simbad

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Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	27.995	62.704	0.334	-1.094	-0.233	–
Chi et al.	2023	27.971	62.722	0.343	-1.098	-0.235	-55.51

💡 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	–	–	–	66	0.120	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CWWDL 2619	35.1	28.3	62.77	0.33	-1.0	-0.28	–	0.3
CWWDL 10632	10.8	28.5	62.85	0.32	-1.0	-0.23	–	0.16
CWWDL 10622	4.1	27.98	63.19	0.33	-1.2	-0.19	–	0.08
Berkeley 7	1.4	28.55	62.37	0.34	-0.98	-0.21	-67.13	0.9
CWWDL 10645	1.4	27.42	62.98	0.29	-0.98	-0.37	-61.0	0.05

💡 Note: The % column shows the percentage of members that CWWDL 2617 shares with each listed object.

Visualization

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