CWNU 2752

0.52 UTI

0.5

C_N

1.0

C_dens

0.62

C_C3

0.25

C_lit

1.0

C_dup

C3 classification CA

Number of members (P>50%) 50

Radius (P>50% members) 5.2 [arcmin]

C_N 0.5 Moderately populated
C_dens 1.0 Very dense
C_C3 0.62 Intermediate quality
C_lit 0.25 Poorly studied
C_dup 1.0 Unique

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

Overview

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CWNU 2752 is a moderately populated, very dense object of intermediate C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster, but with a large variance across recent sources for the age parameter (see Parameters). It was recently reported in the literature.

Relatively close Moderate extinction Near-solar metallicity Young

Cavallo et al. (2024)
Silver sample.

Data

🔍 Search references for CWNU 2752 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	–	221.355	-59.725	0.502	-3.228	-2.194	–
Hunt & Reffert	2024	221.378	-59.698	0.511	-3.204	-2.222	–
Cavallo et al.	2024	221.335	-59.72	0.506	–	–	–
Hunt & Reffert	2023	221.378	-59.698	0.511	-3.204	-2.222	–
He et al.	2023	221.372	-59.721	0.502	-3.232	-2.203	–

💡 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
Hunt & Reffert	2024	–	–	–	–	–	322*	–	–
Cavallo et al.	2024	2.21	2.08	–	468	0.000	–	–	–
Hunt & Reffert	2023	1.86	2.49	2.00	55	–	–	–	–
He et al.	2023	1.86	2.80	–	22	–	–	–	–

(*): Indicates that this parameter is assigned more than one value in the corresponding reference.

Visualization

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