HXHWL 3

0.04 UTI

0.54

C_N

0.21

C_dens

0.75

C_C3

0.0

C_lit

0.14

C_dup

N_m (P>50%) 58

Core radius and density 2.3 [pc], 1.1 [pc^-2]

C3 classification AB

C_N 0.54 Moderately populated
C_dens 0.21 Very loose
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.14 Likely duplicate

📥 Members 📊 Colab 🔬 Bayestar19

MOCA 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

ℹ️

HXHWL 3 is a moderately populated, very loose object of high C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It is rarely studied 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.

Relatively close Low extinction Near-solar metallicity Intermediate age

Data

🔍 Search references for HXHWL 3 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	99999–	115.286	-21.881	0.58	-1.352	1.256	43.452
He et al.	2021	115.274	-21.855	0.55	-1.38	1.24	–

💡 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]	B_frac	BSS
UCC	99999–	1.91	0.76	–	229	0.233	–	–	–
He et al.	2021	1.91	0.76	–	229	0.233	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Teutsch 211	86.2	115.3	-21.88	0.58	-1.36	1.28	44.18	0.38

💡 Note: The % column shows the percentage of members that HXHWL 3 shares with each listed object.

Visualization

ℹ️