CWWDL 2619

0.30 UTI

0.6

C_N

0.17

C_dens

0.75

C_C3

0.0

C_lit

0.99

C_dup

N₅₀ (P>50% members) 70

Stellar density (N₅₀/rad) 0.8 [N/pc²]

C3 classification AB

C_N 0.6 Moderately populated
C_dens 0.17 Very loose
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.99 Unique

📥 Members 📊 Colab 🔬 Bayestar19

MOCA 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

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CWWDL 2619 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 2619 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	99999–	28.304	62.766	0.334	-0.999	-0.28	–
Chi et al.	2023	28.302	62.786	0.337	-1.01	-0.301	-45.453

💡 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]	B_frac	BSS
UCC	99999–	–	–	–	62	0.400	–	–	–
Chi et al.	2023	–	–	–	62	0.400	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CWWDL 2617	37.1	27.99	62.7	0.33	-1.09	-0.23	–	0.3
CWWDL 10632	28.6	28.5	62.85	0.32	-1.0	-0.23	–	0.16
Berkeley 7	1.4	28.55	62.37	0.34	-0.98	-0.21	-67.13	0.9
CWWDL 10622	1.4	27.98	63.19	0.33	-1.2	-0.19	–	0.08

💡 Note: The % column shows the percentage of members that CWWDL 2619 shares with each listed object.

Visualization

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