CWNU 2605

0.35 UTI

0.49

C_N

0.25

C_dens

1.0

C_C3

0.0

C_lit

1.0

C_dup

C3 classification AA

Number of members (P>50%) 49

Radius (P>50% members) 13.1 [arcmin]

C_N 0.49 Poorly populated
C_dens 0.25 Loose
C_C3 1.0 Very high 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 2605 is a poorly populated, loose object of very high C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by very high extinction. It is catalogued as a very young cluster (see Parameters). It was recently reported in the literature.

Note: This object shares a very small percentage of members with a later reported entry. See table with shared members information.

Relatively close Very high extinction Very young

Data

🔍 Search references for CWNU 2605 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	–	307.496	41.513	0.613	-2.446	-2.957	117.607
He et al.	2023	307.645	41.699	0.61	-2.436	-2.902	–

💡 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	1.51	5.75	–	8	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 624	2.0	307.28	41.28	0.59	-2.58	-3.67	-103.5	0.49

💡 Note: The % column shows the percentage of members that CWNU 2605 shares with each listed object.

Visualization

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