CWWDL 14295

0.38 UTI

0.61

C_N

0.62

C_dens

1.0

C_C3

0.0

C_lit

0.85

C_dup

C3 classification AA

Number of members (P>50%) 72

Radius (P>50% members) 19.6 [arcmin]

C_N 0.61 Moderately populated
C_dens 0.62 Moderately dense
C_C3 1.0 Very high quality
C_lit 0.0 Rarely studied
C_dup 0.85 Very likely unique

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

Overview

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CWWDL 14295 is a moderately populated, moderately dense object of very high C3 quality. Its parallax locates it at a close distance, below 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.

Near-solar metallicity Very young

Data

🔍 Search references for CWWDL 14295 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	–	106.331	-27.813	1.185	-3.125	3.396	32.306
Chi et al.	2023	106.435	-27.784	1.193	-3.123	3.416	31.947

💡 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	–	–	–	2	-0.280	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 1913	37.5	106.33	-27.77	1.19	-3.13	3.39	32.81	0.0
OC 0410	15.3	105.73	-27.38	1.2	-3.1	3.48	35.18	0.13

💡 Note: The % column shows the percentage of members that CWWDL 14295 shares with each listed object.

Visualization

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