HXHWL 50

0.02 UTI

0.57

C_N

0.48

C_dens

0.75

C_C3

0.0

C_lit

0.06

C_dup

N_m (P>50%) 64

Core radius and density 1.5 [pc], 2.4 [pc^-2]

C3 classification AB

C_N 0.57 Moderately populated
C_dens 0.48 Loose
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.06 Very likely duplicate

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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HXHWL 50 is a moderately populated, loose object of high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It is rarely studied in the literature.

⚠️ Warning: This is very 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 Moderate extinction Near-solar metallicity Intermediate age

Data

🔍 Search references for HXHWL 50 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	99999–	96.075	7.501	0.495	-0.92	-0.277	46.488
He et al.	2021	96.073	7.5	0.49	-0.9	-0.24	–

💡 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–	2.19	1.27	–	145	0.097	–	–	–
He et al.	2021	2.19	1.27	–	145	0.097	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CWWDL 255	96.9	96.07	7.5	0.5	-0.92	-0.27	46.49	0.02
PHOC 26	93.8	96.07	7.5	0.49	-0.92	-0.28	46.49	0.36

💡 Note: The % column shows the percentage of members that HXHWL 50 shares with each listed object.

Visualization

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