CWWDL 2011

0.06 UTI

0.0

C_N

0.14

C_dens

0.38

C_C3

0.0

C_lit

0.6

C_dup

C3 classification BC

Number of members (P>50%) 17

Radius (P>50% members) 7.6 [arcmin]

C_N 0.0 Sparse
C_dens 0.14 Very loose
C_C3 0.38 Low quality
C_lit 0.0 Rarely studied
C_dup 0.6 Likely unique

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

Overview

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CWWDL 2011 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate distance, near 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 likely a unique object, which shares a moderate 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 2011 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	–	36.345	59.873	0.451	-0.824	-0.543	–
Chi et al.	2023	36.412	59.842	0.47	-0.769	-0.531	–

💡 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	–	–	–	22	0.300	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 1236	40.0	36.27	59.96	0.45	-0.99	-0.56	–	0.11
CWWDL 13770	32.0	36.54	60.02	0.43	-0.65	-0.54	–	0.05
COIN-Gaia 36	28.0	36.3	59.94	0.45	-0.99	-0.56	–	0.64

💡 Note: The % column shows the percentage of members that CWWDL 2011 shares with each listed object.

Visualization

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