CWNU 2275

0.37 UTI

0.75

C_N

0.81

C_dens

0.75

C_C3

0.0

C_lit

0.81

C_dup

C3 classification AB

Number of members (P>50%) 109

Radius (P>50% members) 3.5 [arcmin]

C_N 0.75 Rich
C_dens 0.81 Dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.81 Very likely unique

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

Overview

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CWNU 2275 is a rich, dense object of high C3 quality. Its parallax locates it at a large distance, near the mid-plane, affected by high extinction. It is catalogued as a 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.

Very distant High extinction Very young

Data

🔍 Search references for CWNU 2275 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	–	158.176	-58.625	0.196	-5.471	2.564	85.964
He et al.	2023	158.148	-58.62	0.204	-5.474	2.554	-58.6

💡 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	5.25	4.00	–	4	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
ASCC 60	19.3	158.17	-58.62	0.18	-5.44	2.59	109.42	0.49

💡 Note: The % column shows the percentage of members that CWNU 2275 shares with each listed object.

Visualization

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