CWNU 3605

0.06 UTI

0.56

C_N

1.0

C_dens

1.0

C_C3

0.0

C_lit

0.12

C_dup

C3 classification AA

Number of members (P>50%) 61

Radius (P>50% members) 1.5 [arcmin]

C_N 0.56 Moderately populated
C_dens 1.0 Very dense
C_C3 1.0 Very high quality
C_lit 0.0 Rarely studied
C_dup 0.12 Likely duplicate

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

Overview

ℹ️

CWNU 3605 is a moderately populated, very dense object of very high C3 quality. Its parallax locates it at a moderate^* distance, above the mid-plane, affected by very high extinction. It is catalogued as an intermediate-age cluster (see Parameters). It was recently reported in the literature.

⚠️ Warning: This is likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.

(*): The parallax distance estimate (~4.33 kpc) differs significantly from the median photometric distance (~3.09 kpc).

Distant Very high extinction Intermediate age

Data

🔍 Search references for CWNU 3605 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	141.997	-47.329	0.231	-4.161	3.231	32.651
He et al.	2023	141.994	-47.329	0.25	-4.159	3.236	35.03

💡 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	3.09	5.10	–	398	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 2203	88.5	141.99	-47.33	0.25	-4.16	3.23	30.27	0.5

💡 Note: The % column shows the percentage of members that CWNU 3605 shares with each listed object.

Visualization

ℹ️