CWNU 3460

0.38 UTI

0.27

C_N

1.0

C_dens

0.62

C_C3

0.0

C_lit

1.0

C_dup

C3 classification CA

Number of members (P>50%) 27

Radius (P>50% members) 0.7 [arcmin]

C_N 0.27 Poorly populated
C_dens 1.0 Very dense
C_C3 0.62 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 1.0 Unique

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

Overview

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CWNU 3460 is a poorly populated, very dense object of intermediate C3 quality. Its parallax locates it at a large^* distance, below the mid-plane, affected by moderate extinction. It is catalogued as an intermediate-age cluster (see Parameters). It was recently reported in the literature.

(*): The parallax distance estimate (~5.80 kpc) differs significantly from the median photometric distance (~4.27 kpc).

Distant Moderate extinction Intermediate age

Data

🔍 Search references for CWNU 3460 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	–	7.296	61.127	0.172	-1.31	-0.324	-49.253
He et al.	2023	7.299	61.127	0.178	-1.285	-0.335	-49.25

💡 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
He et al.	2023	4.27	1.80	–	794	–	–	–	–

Visualization

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